<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:wfw="http://wellformedweb.org/CommentAPI/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	xmlns:sy="http://purl.org/rss/1.0/modules/syndication/"
	xmlns:slash="http://purl.org/rss/1.0/modules/slash/"
	xmlns:georss="http://www.georss.org/georss" xmlns:geo="http://www.w3.org/2003/01/geo/wgs84_pos#" xmlns:media="http://search.yahoo.com/mrss/"
	>

<channel>
	<title>A Quantum Diaries Survivor &#187; Tevatron</title>
	<atom:link href="http://dorigo.wordpress.com/tag/tevatron/feed/" rel="self" type="application/rss+xml" />
	<link>http://dorigo.wordpress.com</link>
	<description>private thoughts of a physicist and chessplayer</description>
	<lastBuildDate>Mon, 05 Oct 2009 19:39:35 +0000</lastBuildDate>
	<generator>http://wordpress.com/</generator>
	<language>en</language>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
	<cloud domain='dorigo.wordpress.com' port='80' path='/?rsscloud=notify' registerProcedure='' protocol='http-post' />
<image>
		<url>http://www.gravatar.com/blavatar/ea8680268b387234a38cc9325db0f57d?s=96&#038;d=http://s.wordpress.com/i/buttonw-com.png</url>
		<title>A Quantum Diaries Survivor &#187; Tevatron</title>
		<link>http://dorigo.wordpress.com</link>
	</image>
	<atom:link rel="search" type="application/opensearchdescription+xml" href="http://dorigo.wordpress.com/osd.xml" title="A Quantum Diaries Survivor" />
		<item>
		<title>Just a link</title>
		<link>http://dorigo.wordpress.com/2009/04/05/just-a-link/</link>
		<comments>http://dorigo.wordpress.com/2009/04/05/just-a-link/#comments</comments>
		<pubDate>Sun, 05 Apr 2009 21:34:14 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[Blogroll]]></category>
		<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[science reporting]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2241</guid>
		<description><![CDATA[I read with amusement (and some effort) a spanish account by Francis (th)E mule of Michael Dittmar&#8217;s controversial seminar of last March 19th. I paste the link here for several reasons: since I believe it might be of interest to some of you, to have a place to store it, and because I am not [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2241&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>I read with amusement (and some effort) a spanish account by <a href="http://francisthemulenews.wordpress.com/">Francis (th)E mule</a> of Michael Dittmar&#8217;s <a href="http://dorigo.wordpress.com/2009/03/20/a-seminar-against-the-tevatron/">controversial seminar</a> of last March 19th. I paste the link <a href="http://francisthemulenews.wordpress.com/2009/04/05/dorigo-contra-dittmar-un-combate-de-boxeo-dialectico-contra-el-tevatron-en-el-cern/">here</a> for several reasons: since I believe it might be of interest to some of you, to have a place to store it, and because I am not insensitive to flattery:</p>
<blockquote><p>&#8220;Entre el público se encontraba  Tomasso Dorigo [...] (r)esponsable del mejor blog sobre física de partículas elementales del mundo&#8221;</p></blockquote>
<p>Muchas gracias, Francis -but please note: my name spells with two m&#8217;s and one s!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2241/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2241/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2241/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2241/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2241/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2241/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2241/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2241/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2241/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2241/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2241&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/04/05/just-a-link/feed/</wfw:commentRss>
		<slash:comments>10</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>Latest global fits to SM observables: the situation in March 2009</title>
		<link>http://dorigo.wordpress.com/2009/03/25/latest-global-fits-to-sm-observables-the-situation-in-march-2009/</link>
		<comments>http://dorigo.wordpress.com/2009/03/25/latest-global-fits-to-sm-observables-the-situation-in-march-2009/#comments</comments>
		<pubDate>Wed, 25 Mar 2009 12:44:16 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[electroweak fits]]></category>
		<category><![CDATA[Gfitter]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LEP]]></category>
		<category><![CDATA[SLD]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top quark]]></category>
		<category><![CDATA[W boson]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2216</guid>
		<description><![CDATA[A recent discussion in this blog between well-known theorists and phenomenologists, centered on the real meaning of the experimental measurements of top quark and W boson masses, Higgs boson cross-section limits, and other SM observables, convinces me that some clarification is needed.
The work has been done for us: there are groups that do exactly that, [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2216&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>A recent discussion in this blog between well-known theorists and phenomenologists, centered on the real meaning of the experimental measurements of top quark and W boson masses, Higgs boson cross-section limits, and other SM observables, convinces me that some clarification is needed.</p>
<p>The work has been done for us: there are groups that do exactly that, i.e. updating their global fits to express the internal consistency of all those measurements, and the implications for the search of the Higgs boson. So let me go through the most important graphs below, after mentioning that most of the material comes from the <a href="http://lepewwg.web.cern.ch/LEPEWWG/">LEP electroweak working group web site</a>.</p>
<p>First of all, what goes in the soup ? Many things, but most notably, the LEP I/SLD measurements at the Z pole, the top quark mass measurements by CDF and DZERO, and the W mass measurements by CDF, DZERO, and LEP II. Let us give a look at the mass measurements, which have recently been updated.</p>
<p>For the top mass, the situation is the one pictured in the graph shown below. As you can clearly see, the CDF and DZERO measurements have reached a combined precision of 0.75% on this quantity.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/mt09.jpg" alt="" width="460" /></p>
<p>The world average is now at <img src='http://l.wordpress.com/latex.php?latex=M_t+%3D+173.1+%5Cpm+1.3+GeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_t = 173.1 \pm 1.3 GeV' title='M_t = 173.1 \pm 1.3 GeV' class='latex' />. I am amazed to see that the first estimate of the top mass, made by a handful of events <a href="http://www-cdf.fnal.gov/physics/preprints/cdf2595_top_prl.ps.gz">published by CDF in 1994</a> (a set which did not even provide a conclusive &#8220;observation-level&#8221; significance at the time) was so dead-on: the measurement back then was <img src='http://l.wordpress.com/latex.php?latex=M_t%3D174+%5Cpm+15+GeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_t=174 \pm 15 GeV' title='M_t=174 \pm 15 GeV' class='latex' />! (for comparison, the DZERO measurement of 1995, in their <a href="http://www-d0.fnal.gov/www_buffer/pub/pub_007.pdf">&#8220;observation&#8221; paper</a>, was <img src='http://l.wordpress.com/latex.php?latex=M_t%3D199+%5Cpm+30+GeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_t=199 \pm 30 GeV' title='M_t=199 \pm 30 GeV' class='latex' />).</p>
<p>As far as global fits are concerned, there is one additional point to make for the top quark: knowing the top mass any better than this has become, by now, useless. You can see it by comparing the constraints on <img src='http://l.wordpress.com/latex.php?latex=M_t&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_t' title='M_t' class='latex' /> coming from the indirect measurements and W mass measurements (shown by the blue bars at the bottom of the graph above) with the direct measurements at the Tevatron (shown with the green band). The green band is already too narrow: the width of the blue error bars compared to the narrow green band tells us that the SM does not care much where exactly the top mass is, by now.</p>
<p>Then, let us look at the W mass determinations. Note, the graph below shows the situation <strong>BEFORE </strong>the <a href="http://www-d0.fnal.gov/Run2Physics/WWW/results/prelim/EW/E27/E27.pdf">latest DZERO result</a>;, obtained with 1/fb of data, and which finds <img src='http://l.wordpress.com/latex.php?latex=M_W+%3D+80401+%5Cpm+44+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_W = 80401 \pm 44 MeV' title='M_W = 80401 \pm 44 MeV' class='latex' />; its inclusion would not change much of the discussion below, but it is important to stress it.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/mw09.jpg" alt="" width="460" /></p>
<p>Here the situation is different: a better measurement would still increase the precision of our comparisons with indirect information from electroweak measurements at the Z. This is apparent by observing that the blue bars have width still smaller than the world average of direct measurements (again in green). Narrow the green band, and you can still collect interesting information on its consistency with the blue points.</p>
<p>Finally, let us look at the global fit: the electroweak working group at LEP displays in the by now famous &#8220;blue band plot&#8221;, shown below for March 2009 conferences. It shows the constraints on the Higgs boson mass coming from all experimental inputs combined, assuming that the Standard Model holds.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/blueband.jpg" alt="" width="460" /></p>
<p>I will not discuss this graph in details, since I have done it repeatedly in the past. I will just mention that the yellow regions have been excluded by direct searches of the Higgs boson at LEP II (on the left, the wide yellow area) and the Tevatron ( the narrow strip on the right). From the plot you should just gather that a light Higgs mass is preferred (the central value being 90 GeV, with +36 and -27 GeV one-sigma error bars). Also, a 95% confidence-level exclusion of masses above 163 GeV is implied by the variation of the global fit <img src='http://l.wordpress.com/latex.php?latex=%5Cchi%5E2&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\chi^2' title='\chi^2' class='latex' /> with Higgs mass.</p>
<p>I have started to be a bit bored by this plot, because it does not do the best job for me. For one thing,<span style="color:#ff0000;"> the LEP II limit and the Tevatron limit on the Higgs mass are treated as if they were equivalent in their strength</span>, something which could not be possibly farther from the truth. The truth is, the LEP II limit is a very strong one -the probability that the Higgs has a mass below 112 GeV, say, is one in a billion or so-, while the limit obtained recently by the Tevatron is just an &#8220;indication&#8221;, because the excluded region (160 to 170 GeV) is not excluded strongly: there still is a one-in-twenty chance or so that the real Higgs boson mass indeed lies there.</p>
<p>Another thing I do not particularly like in the graph is that <span style="color:#3366ff;">it attempts to pack too much information</span>: variations of <img src='http://l.wordpress.com/latex.php?latex=%5Calpha&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\alpha' title='\alpha' class='latex' />, inclusion of low-Q^2 data, etcetera. A much better graph to look at is the one produced by the GFitter group instead. It is shown below.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/gfitter09.jpg" alt="" width="460" /></p>
<p>In this plot, the direct search results are introduced with their actual measured probability of exclusion as a function of Higgs mass, and not just in a digital manner, yes/no, as the yellow regions in the blue band plot. And in fact, you can see that the LEP II limit is a brick wall, while the Tevatron exclusion acts like a smooth increase in the global <img src='http://l.wordpress.com/latex.php?latex=%5Cchi%5E2&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\chi^2' title='\chi^2' class='latex' /> of the fit.</p>
<p>From the black curve in the graph you can get a lot of information. For instance, <span style="color:#ff0000;">the most likely values, those that globally have a 1-sigma probability of being one day proven correct, are masses contained in the interval 114-132 GeV</span>. At two-sigma, the Higgs mass is instead within the interval 114-152 GeV, and at three sigma, it extends into the Tevatron-excluded band a little, 114-163 GeV, with a second region allowed between 181 and 224 GeV.</p>
<p>In conclusion, I would like you to take away the following few points:</p>
<ul>
<li>Future indirect constraints on the Higgs boson mass will only come from increased precision measurements of the W boson mass, while the top quark has exhausted its discrimination power;</li>
<li>Global SM fits show an overall very good consistency: there does not seem to be much tension between fits and experimental constraints;</li>
<li>The Higgs boson is most likely in the 114-132 GeV range (1-sigma bounds from global fits).</li>
</ul>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2216/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2216/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2216/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2216/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2216/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2216/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2216/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2216/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2216/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2216/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2216&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/25/latest-global-fits-to-sm-observables-the-situation-in-march-2009/feed/</wfw:commentRss>
		<slash:comments>18</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/mt09.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/mw09.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/blueband.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/gfitter09.jpg" medium="image" />
	</item>
		<item>
		<title>Zooming in on the Higgs</title>
		<link>http://dorigo.wordpress.com/2009/03/24/zooming-in-on-the-higgs/</link>
		<comments>http://dorigo.wordpress.com/2009/03/24/zooming-in-on-the-higgs/#comments</comments>
		<pubDate>Tue, 24 Mar 2009 13:04:07 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LEP]]></category>
		<category><![CDATA[MSSM]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[supersymmetry]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top quark]]></category>
		<category><![CDATA[W boson]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2213</guid>
		<description><![CDATA[Yesterday Sven Heinemeyer kindly provided me with an updated version of a plot which best describes the experimental constraints on the Higgs boson mass, coming from electroweak observables measured at LEP and SLD, and from the most recent measurements of W boson and top quark masses. It is shown on the right (click to get [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2213&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><a href="http://www.pd.infn.it/~dorigo/mwmt_sven_09_large.jpg"><img class="alignright" src="http://www.pd.infn.it/~dorigo/mwmt_sven_09_small.jpg" alt="" /></a>Yesterday <a href="http://www.ifca.unican.es/~heinemey/uni/plots/">Sven Heinemeyer</a> kindly provided me with an updated version of a plot which best describes the experimental constraints on the Higgs boson mass, coming from electroweak observables measured at LEP and SLD, and from the most recent measurements of W boson and top quark masses. It is shown on the right (click to get the full-sized version).</p>
<p>The graph is a quite busy one, but I will try below to explain everything one bit at a time, hoping I keep things simple enough that a non-physicist can understand it.</p>
<p>The axes show suitable ranges of values of the top quark mass (varying on the horizontal axis) and of the W boson masses (on the vertical axis). The value of these quantities is functionally dependent (because of quantum effects connected to the propagation of the particles and their interaction with the Higgs field) on the Higgs boson mass.</p>
<p>The dependence, however, is really &#8220;soft&#8221;: if you were to double the Higgs mass by a factor of two from its true value, the effect on top and W masses would be only of the order of 1% or less. Because of that, only recently have the determinations of top quark and W boson masses started to provide meaningful inputs for a guess of the mass of the Higgs.</p>
<p>Top mass and W mass measurements are plotted in the graphs in the form of ellipses encompassing the most likely values: their size is such that the true masses should lie within their boundaries, 68% of the time. The red ellipse shows CDF results, and the blue one shows DZERO results.</p>
<p><img class="alignright" src="http://www.pd.infn.it/~dorigo/mwmt_sven_09_mw.jpg" alt="" width="300" />There is a third measurement of the W mass shown in the plot: it is displayed as a horizontal band limited by two black lines, and it comes from the LEP II measurements. The band also encompasses the 68% most likely W masses, as ellipses do.</p>
<p>In addition to W and top masses, other experimental results constrain the mass of top, W, and Higgs boson. The most stringent of these results are those coming from the LEP experiment at CERN, from detailed analysis of electroweak interactions studied in the production of Z bosons. A wide band crossing the graph from left to right, with a small tilt, encompasses the most likely region for top and W masses.</p>
<p><img class="alignright" src="http://www.pd.infn.it/~dorigo/mwmt_sven_09_mh.jpg" alt="" />So far we have described measurements. Then, there are two different physical models one should consider in order to link those measurements to the Higgs mass. The first one is the Standard Model: it dictates precisely the inter-dependence of all the parameters mentioned above. Because of the precise SM predictions, for any choice of the Higgs boson mass one can draw a curve in the top mass versus W mass plane. However, in the graph a full band is hatched instead. This correspond to allowing the Higgs boson mass to vary from a minimum of 114 GeV to 400 GeV. 114 GeV is the lower limit on the Higgs boson mass found by the LEP II experiments in their direct searches, using electron-positron collisions; while 400 GeV is just a reference value.</p>
<p>The boundaries of the red region show the functional dependence of Higgs mass on top and W masses: an increase of top mass, for fixed W mass, results in an increase of the Higgs mass, as is clear by starting from the 114 GeV upper boundary of the red region, since one then would move into the region, to higher Higgs masses. On the contrary, for a fixed top mass, an increase in W boson mass results in a decrease of the Higgs mass predicted by the Standard Model. Also note that the red region includes a narrow band which has been left white: it is the region corresponding to Higgs masses varying between 160 and 170 GeV, the masses that direct searches at the Tevatron have excluded at 95% confidence level.</p>
<p><img class="alignright" src="http://www.pd.infn.it/~dorigo/mwmt_sven_09_mssm.jpg" alt="" />The second area, hatched in green, is not showing a single model predictions, but rather a range of values allowed by varying arbitrarily many of the parameters describing the supersymmetric extension of the SM called &#8220;MSSM&#8221;, its &#8220;minimal&#8221; extension. Even in the minimal extension there are about a hundred additional parameters introduced in the theory, and the values of a few of those modify the interconnection between top mass and W mass in a way that makes direct functional dependencies in the graph impossible to draw. Still, the hatched green region shows a &#8220;possible range of values&#8221; of the top quark and W boson masses. The arrow pointing down only describes what is expected for W and top masses if the mass of supersymmetric particles is increased from values barely above present exclusion limits to very high values.</p>
<p>So, to summarize, what to get from the plot ? I think the graph describes many things in one single package, and it is not easy to get the right message from it alone. Here is a short commentary, in bits.</p>
<ul>
<li>All experimental results are consistent with each other (but here, I should add, a result from NuTeV which finds indirectly the W mass from the measured ratio of neutral current and charged current neutrino interactions is not shown);</li>
<li>Results point to a small patch of the plane, consistent with a light Higgs boson if the Standard Model holds</li>
<li>The lower part of the MSSM allowed region is favored, pointing to heavy supersymmetric particles if that theory holds</li>
<li>Among experimental determinations, the most constraining are those of the top mass; but once the top mass is known to within a few GeV, it is the W mass the one which tells us more about the unknown mass of the Higgs boson</li>
<li>One point to note when comparing measurements from LEP II and the Tevatron experiments: when one draws a 2-D ellipse of 68% contour, this compares unfavourably to a band, which encompasses the same probability in a 1-D distribution. This is clear if one compares the actual measurements: CDF <img src='http://l.wordpress.com/latex.php?latex=80.413+%5Cpm+48+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='80.413 \pm 48 MeV' title='80.413 \pm 48 MeV' class='latex' /> (with 200/pb of data), DZERO <img src='http://l.wordpress.com/latex.php?latex=80%2C401+%5Cpm+44+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='80,401 \pm 44 MeV' title='80,401 \pm 44 MeV' class='latex' /> (with five times more statistics), LEP II <img src='http://l.wordpress.com/latex.php?latex=80.376+%5Cpm+33+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='80.376 \pm 33 MeV' title='80.376 \pm 33 MeV' class='latex' /> (average of four experiments). The ellipses look like they are half as precise as the black band, while they are actually only 30-40% worse. If the above is obscure to you, a simple graphical explanation is provided <a href="http://dorigo.wordpress.com/2008/05/14/updated-mw-mt-higgs-search-plot-from-sven/">here</a>.</li>
<li>When averaged, CDF and DZERO will actually beat the LEP II precision measurement -and they are sitting on 25 times more data (CDF) or 5 times more (DZERO).</li>
</ul>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2213/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2213/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2213/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2213/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2213/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2213/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2213/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2213/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2213/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2213/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2213&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/24/zooming-in-on-the-higgs/feed/</wfw:commentRss>
		<slash:comments>27</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/mwmt_sven_09_small.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/mwmt_sven_09_mw.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/mwmt_sven_09_mh.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/mwmt_sven_09_mssm.jpg" medium="image" />
	</item>
		<item>
		<title>A seminar against the Tevatron!</title>
		<link>http://dorigo.wordpress.com/2009/03/20/a-seminar-against-the-tevatron/</link>
		<comments>http://dorigo.wordpress.com/2009/03/20/a-seminar-against-the-tevatron/#comments</comments>
		<pubDate>Fri, 20 Mar 2009 17:37:28 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LHC]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2200</guid>
		<description><![CDATA[I spent this week at CERN to attend the meetings of the CMS week &#8211; an event which takes place four times a year, when collaborators of the CMS experiment, coming from all parts of the world, get together at CERN  to discuss detector commissioning, analysis plans, and recent results. It was a very [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2200&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>I spent this week at CERN to attend the meetings of the CMS week &#8211; an event which takes place four times a year, when collaborators of the CMS experiment, coming from all parts of the world, get together at CERN  to discuss detector commissioning, analysis plans, and recent results. It was a very busy and eventful week, and only now, sitting on a train that brings me back from Geneva to Venice, can I find the time to report with the due dedication on some things you might be interested to know about.</p>
<p>One thing to report on is certainly the seminar I eagerly attended on Thursday morning, by Michael Dittmar (ETH-Zurich). Dittmar is a CMS collaborator, and he talked at the CERN theory division on a tickling subject:&#8221;Why I never believed in the Tevatron Higgs sensitivity claims for Run 2ab&#8221;. The title did promise a controversial discussion, but I was really startled by its level, as much as by the defamation of which I felt personally to be a target. I will explain this below.</p>
<p>I have also to mention that by Thursday I had already attended to a reduced version of his talk, since he had given it on the previous day in another venue. Both I and John Conway had corrected him on a few plainly wrong statements back then, but I was puzzled to see he reiterated those false statements in the longer seminar! More on that below.</p>
<p><strong>Dittmar&#8217;s obnoxious seminar<br />
</strong></p>
<p>Dittmar started by saying he was infuriated by the recent BBC article where &#8220;a statement from the director of a famous laboratory&#8221; claimed that the Tevatron had 50% odds of finding a Higgs boson, in a certain mass range. This prompted him to prepare a seminar to express his scepticism. However, <span style="color:#3366ff;">it turned out that his scepticism was not directed solely at the optimistic statement he had read, but at every single result on Higgs searches that CDF and DZERO had produced since Run I.</span></p>
<p>In order to discuss sensitivity and significances, the speaker made a un-illuminating digression on how counting experiments can or cannot obtain observation-level significances with their data depending on the level of background of their searches and the associated systematical uncertainties. His statements were very basic and totally uncontroversial on this issue, but he failed to focus on the fact that nowadays, nobody does counting experiments any more when searching for evidence of a specific model: our confidence in advanced analysis methods involving neural networks, shape analysis, and likelihood discriminants; the tuning of Monte Carlo simulations; and the accurate analytical calculations of high-order diagrams for Standard Model processes, have all grown tremendously with years of practice and studies, and these methods and tools overcome the problems of searches for small signals immersed in large backgrounds. One can be sceptical, but one cannot ignore the facts, as the speaker seemed inclined to.</p>
<p>Then Dittmar said that in order to judge the value of sensitivity claims for the future, one may turn to past studies and verify their agreement with the actual results. So he turned to the Tevatron Higgs Sensitivity studies of 2000 and 2003, two endeavours to which I had participated with enthusiasm.</p>
<p>He produced a plot showing the small signal of <img src='http://l.wordpress.com/latex.php?latex=ZH+%5Cto+l%5E%2B+l%5E-+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='ZH \to l^+ l^- b \bar b' title='ZH \to l^+ l^- b \bar b' class='latex' /> decays that the Tevatron 2000 study believed the two experiments could achieve with 10 inverse femtobarns of data, expressing his doubts that the &#8220;tiny excess&#8221; could mean an evidence for Higgs production. On the side of that graph, he had for comparison placed a result of CDF on real Run I data, where a signal of WH or ZH decays to four jets had been searched in the dijet invariant mass distribution of the two b-jets.</p>
<p><span style="color:#ff0000;">He commented that figure by saying half-mockingly that the data could have been used to exclude the standard model process of associated <img src='http://l.wordpress.com/latex.php?latex=Z%2Bjets&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Z+jets' title='Z+jets' class='latex' /> production, since the contribution from Z decays to b-quark pairs was sitting at a mass where one bin had fluctuated down by two standard deviations with respect to the sum of background processes. </span>This ridiculous claim was utterly unsupported by the plot -which had an overall very good agreement between data and MC sources- and by the fact that the bins adjacent to the downward-fluctuating one were higher than the prediction. I found this claim really disturbing, because it tried to denigrate my experiment with a futile and incorrect argument. <span style="color:#3366ff;">But I was about to get more upset for his next statement.</span></p>
<p>In fact, he went on to discuss the global expectation of the Tevatron on Higgs searches, a graph (see below) produced in 2000 after a big effort from several tens of people in CDF and DZERO.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/tev_hreach_98.jpg" alt="" width="460" /></p>
<p>He started by saying that the graph was confusing, and that it was not clear in the documentation how it had been produced, nor that it was the combination of CDF and DZERO sensitivity. This was very amusing, since sitting from the far back John Conway, a CDF colleague, shouted: &#8220;It says it in print on top of it: combined thresholds!&#8221;, then adding, with a pacate voice &#8220;&#8230;In case you&#8217;re wondering, I made that plot.&#8221; John had in fact been the leader of the Tevatron Higgs sensitivity study, not to mention the author of many of the most interesting searches for the higgs boson in CDF since then.</p>
<p>Dittmar continued his surreal talk with an overbid, by <span style="color:#ff0000;">claiming that the plot had been produced &#8220;by assuming a 30% improvement in the mass resolution of pairs of b-jets, when nobody had not even the least idea on how such improvement could be achieved&#8221;.</span></p>
<p>I could not have put together a more personal, direct attack to years of my own work myself! It is no mystery that I worked on dijet resonances since 1992, but of course I am a rather unknown soldier in this big game; however, I felt the need to interrupt the speaker at this point -exactly as I had done at the shorter talk the day before.</p>
<p>I remarked that in 1998, one year before the Tevatron sensitivity study, I had produced a PhD thesis and public documents showing the observation of a signal of <img src='http://l.wordpress.com/latex.php?latex=Z+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Z \to b \bar b' title='Z \to b \bar b' class='latex' /> decays in CDF Run I data, and had demonstrated on that very signal how the use of ingenuous algorithms could reduce by at least 30% the dijet mass resolution, making the signal more prominent. The relevant plots are below, directly from my PhD thesis: judge for yourself.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/zbbmc1.jpg" alt="" width="460" /></p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/zbbmc2.jpg" alt="" width="460" /></p>
<p>In the plots, you can see how <span style="color:#3366ff;">the excess over background predictions moves to the right as more and more refined jet energy corrections are applied, starting from the result of generic jet energy corrections (top) to optimized corrections (bottom) until the signal becomes narrower and centered at the true value</span>. The plots on the left show the data and the background prediction, those on the right show the difference, which is due to Z decays to b-quark jet pairs. Needless to say, the optimization is done on Monte Carlo Z events, and only then checked on the data.</p>
<p>So I said that Dittmar&#8217;s statement was utterly false: we had an idea of how to do it, we had proven we could do it, and besides, the plots showing what we had done had been indeed included in the Tevatron 2000 report. Had he overlooked them ?</p>
<p><strong>Escalation!<br />
</strong></p>
<p>Dittmar seemed unbothered by my remark, and he responded that that small signal had not been confirmed in Run II data. His statement constituted an even more direct attack to four more years of my research time, spent on that very topic. I kept my cool, because when your opponent offers you on a silver plate the chance to verbally sodomize him, you cannot be too angry with him.</p>
<p>I remarked that a signal had indeed been found in Run II, amounting to about 6000 events after all selection cuts; it confirmed the past results. Dittmar then said that <span style="color:#3366ff;">&#8220;to the best of his knowledge&#8221; this had not been published, so it did not really count. </span><span style="color:#ff0000;">I then explained it was a 2008 NIM publication, and would he please document himself before making such unsubstantiated allegations? </span>He shrugged his shoulders, said he would look more carefully for the paper, and went back to his talk.</p>
<p><img class="alignleft" src="http://www.pd.infn.it/~dorigo/cdf_higgs_reach_09.jpg" alt="" width="200" /> His points about the Tevatron sensitivity studies were laid down: for a low-mass Higgs boson, the signal is just too small and backgrounds are too large, and the sensitivity of real searches is below expectations by a large factor. <span style="color:#ff0000;">To stress this point, he produced a slide containing a plot he had taken from this blog! </span>The plot (see on the left), which is my own concoction and not Tevatron-approved material, shows the ratio between observed limit to Higgs production and the expectations of the 2000 study. He pointed at the two points for 100-140 GeV Higgs boson masses, trying to prove his claim: The Tevatron is now doing three times worse than expected. He even uttered &#8220;<span style="text-decoration:underline;">It is time to confess: the sensitivity study was wrong by a large factor!&#8221;.</span></p>
<p>I could not help interrupting again: I had to stress that the plot was not approved material and was just a private interpretation of Tevatron results, but I did not deny its contents. The plot was indeed showing that low-mass searches were below par, but it was also showing that high-mass ones were amazingly in agreement with expectations worked at 10 years before. Then John Conway explained the low-mass discrepancy for the benefit of the audience, as he had done one day before for no apparent benefit of the speaker.</p>
<p><span style="color:#3366ff;">Conway explained that the study had been done under the hypothesis that an upgrade of our silicon detector would be financed by the DoE: it was in fact meant to prove the usefulness of funding an upgrade</span>. A larger acceptance of inner silicon tracking boosts the sensitivity to identify b-quark jets from Higgs decays by a large factor, because any acceptance increase gets squared when computing the over-efficiency. So Dittmar could not really blame the Tevatron experiments for predicting something that would not materialize in a corresponding result, given that the DoE had denied the funding to build the upgraded detector!</p>
<p>I then felt compelled to add that by using my plot Dittmar was proving the opposite thesis of what he wanted to demonstrate: low-mass Tevatron searches were shown to underperform because of funding issues, rather than because of a wrong estimate of sensitivity; and high-mass searches, almost unhindered by the lack of an upgraded silicon, were in excellent agreement with expectations!</p>
<p>The speaker said that no, the high-mass searches were not in agreement, because their results could not be believed, and moved on to discuss those by taking real-data results by the Tevatron.</p>
<p>He said that the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+WW&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to WW' title='H \to WW' class='latex' /> is a great channel at the LHC.</p>
<blockquote><p>&#8220;Possible at the Tevatron ? I believe that the WW continuum background is much larger at a ppbar collider than at a pp collider, so my personal conclusion is that if the Tevatron people want to waste their time on it, good luck to them.&#8221;</p></blockquote>
<p>Now, come on. I cannot imagine how a respectable particle physicist could drive himself into making such statements in front of a distinguished audience (which, have I mentioned it, included several theorists of the highest caliber, including none less than <span style="color:#ff0000;">Edward Witten</span>). Waste their time ? I felt I was wasting my time listening to him, but my determination of reporting his talk here kept me anchored to my chair, taking notes.</p>
<p>So this second part of the talk was not less unpleasant than the first part: Dittmar criticized the Tevatron high-mass Higgs results in the most incorrect, and scientifically dishonest, way that I could think of. Here is just a summary:</p>
<ul>
<li>He picked up a distribution of one particular sub-channel from one experiment, noting that it seemed to have the most signal-rich region showing a deficit of events. He then showed the global CDF+DZERO limit, which did not show a departure between expected and observed limit on Higgs cross section, and concluded that there was something fishy in the way the limit had been evaluated. But the limit is extracted from literally several dozens of those distributions -something he failed to mention despite having been warned of that very issue in advance.</li>
</ul>
<ul>
<li>He picked up two neural-network output distributions for a search of Higgs at 160 and 165 GeV, and declared they could not be correct since they were very different in shape! John, from the back, replied &#8220;You have never worked with neural networks, have you ?&#8221; No, he had not. Had he, he would probably have understood that different mass points, optimized differently, can provide very different NN outputs.</li>
</ul>
<ul>
<li>He showed another Neural Network output based on 3/fb of data, which had a pair of data points lying one standard deviation above the background predictions, and the corresponding plot for a search performed with improved statistics, which had instead a underfluctuation. He said he was puzzled by the effect. Again, some intervention from the audience was necessary, explaining that the methods are constantly reoptimized, and there is no wonder that adding more data can result in a different outcome. This produced a discussion when somebody from the audience tried to speculate that searches were maybe performed by looking at the data before choosing which method to use for a limit extraction! On the contrary of course, all Tevatron searches of the Higgs are blind analyses, where the optimization is performed on expected limits, using control samples, and Monte Carlo, and the data is only looked at afterwards.</li>
<li>He showed that the Tevatron 2000 report had estimated a maximum Signal/Noise ratio for the H&#8211;&gt;WW search of 0.34, and he picked up one random plot from the many searches of that channel by CDF and DZERO, showing that the signal to noise there was never larger than 0.15 or so. Explaining to him that the S/N of searches based on neural networks and combined discriminants is not a fixed value, and that many improvements have occurred in data analysis techniques in 10 years was useless.</li>
</ul>
<p>Dittmar concluded his talk by saying that:</p>
<blockquote><p>&#8220;Optimistic expectations might help to get funding! This is true, but it is also true that this approach eventually destroys some remaining confidence in science of the public.&#8221;.</p></blockquote>
<p>His last slide even contained the sentence he had previously brought himself to uttering:</p>
<blockquote><p>&#8220;It is the time to confess and admit that the sensitivity predictions were wrong&#8221;.</p></blockquote>
<p>Finally, <span style="color:#ff0000;">he encouraged LHC experiments to looking for the Higgs where the Tevatron had excluded it</span> -between 160 and 170 GeV- because Tevatron results cannot be believed. I was disgusted: he most definitely places a strong claim on the prize of the most obnoxious talk of the year. Unfortunately for all, it was just as much an incorrect, scientifically dishonest, and dilettantesque lamentation, plus a defamation of a community of 1300 respected physicists.</p>
<p>In the end, I am really wondering what really moved Dittmar to such a disastrous performance. I think I know the answer, at least in part: he has been an advocate of the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+WW&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to WW' title='H \to WW' class='latex' /> signature since 1998, and he must now feel bad for that beautiful process being proven hard to see, by his &#8220;enemies&#8221;. Add to that the frustration of seeing the Tevatron producing brilliant results and excellent performances, while CMS and Atlas are sitting idly in their caverns, and you might figure out there is some human factor to take into account. But nothing, in my opinion, can justify the mix he put together: false allegations, disregard of published material, manipulation of plots, public defamation of respected colleagues. I am sorry to say it, but even though I have nothing personal against Michael Dittmar -I do not know him, and in private he might even be a pleasant person-, it will be very difficult for me to collaborate with him for the benefit of the CMS experiment in the future.</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2200/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2200/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2200/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2200/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2200/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2200/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2200/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2200/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2200/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2200/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2200&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/20/a-seminar-against-the-tevatron/feed/</wfw:commentRss>
		<slash:comments>56</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/tev_hreach_98.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/zbbmc1.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/zbbmc2.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/cdf_higgs_reach_09.jpg" medium="image" />
	</item>
		<item>
		<title>Streaming video for Y(4140) discovery</title>
		<link>http://dorigo.wordpress.com/2009/03/17/streaming-video-for-y4140-discovery/</link>
		<comments>http://dorigo.wordpress.com/2009/03/17/streaming-video-for-y4140-discovery/#comments</comments>
		<pubDate>Tue, 17 Mar 2009 18:15:23 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[B physics]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[discoveries]]></category>
		<category><![CDATA[QCD]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2189</guid>
		<description><![CDATA[The CDF collaboration will present at a public venue (Fermilab&#8217;s Wilson Hall) its discovery of the new Y(4140) hadron, a mysterious particle created in B meson decays, and observed to decay strongly into a  state, a pair of vector mesons. I have described that exciting discovery in a recent post.
From this site you can [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2189&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>The CDF collaboration will present at a public venue (Fermilab&#8217;s Wilson Hall) its discovery of the new Y(4140) hadron, a mysterious particle created in B meson decays, and observed to decay strongly into a <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi+%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi \phi' title='J/\psi \phi' class='latex' /> state, a pair of vector mesons. I have described that exciting discovery <a href="http://dorigo.wordpress.com/2009/03/13/cdf-discovers-a-new-hadron/">in a recent post</a>.</p>
<p><a href="http://vms-db-srv.fnal.gov/fmi/xsl/VMS_Site_2/000Return/video/r_livelogicindex.xsl?&amp;-recid=481&amp;-find=">From this site</a> you can connect to streaming video (starting at 4.00PM CDT, or 9.00PM GMT &#8211; should last about 1.30 hours).</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2189/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2189/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2189/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2189/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2189/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2189/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2189/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2189/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2189/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2189/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2189&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/17/streaming-video-for-y4140-discovery/feed/</wfw:commentRss>
		<slash:comments>1</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>DZERO refutes CDF&#8217;s multimuon signal&#8230; Or does it ?</title>
		<link>http://dorigo.wordpress.com/2009/03/17/dzero-refutes-cdfs-multimuon-signal-or-does-it/</link>
		<comments>http://dorigo.wordpress.com/2009/03/17/dzero-refutes-cdfs-multimuon-signal-or-does-it/#comments</comments>
		<pubDate>Tue, 17 Mar 2009 14:43:48 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[anomalous muons]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[new physics]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2184</guid>
		<description><![CDATA[Hot off the press: Mark Williams, a DZERO member speaking at Moriond QCD 2009 -a yearly international conference in particle physics, where HEP experimentalists regularly present their hottest results- has shown today the preliminary results of their analysis of dimuon events, based on 900 inverse picobarns of proton-antiproton collision data. And the conclusion is&#8230;
DZERO searched [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2184&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Hot off the press: Mark Williams, a DZERO member speaking at Moriond QCD 2009 -a yearly international conference in particle physics, where HEP experimentalists regularly present their hottest results- has shown today the <a href="http://moriond.in2p3.fr/QCD/2009/TuesdayMorning/Williams.pdf">preliminary results</a> of their analysis of dimuon events, based on 900 inverse picobarns of proton-antiproton collision data. And the conclusion is&#8230;</p>
<p>DZERO searched for an excess of muons with large impact parameter by applying a data selection very similar, and when possible totally equivalent, to the one used by CDF in its recent study. Of course, the two detectors have entirely different hardware, software algorithms, and triggers, so there are certain limits to how closely one analysis can be replicated by the other experiment. However, the main machinery is quite similar: they count how many events have two muons produced within the first layer of silicon detector, and extrapolate to determine how many they expect to see which fail to yield a hit in that first layer, comparing to the actual number. <em>They find no excess of large impact parameter muons</em>.</p>
<p><span style="color:#ff0000;">Impact parameter</span>, for those of you who have not followed this closely in the last few months, is the smallest distance between a track and the proton-antiproton collision vertex, in the plane transverse to the beam direction. A large impact parameter indicates that a particle has been produced in the decay of a parent body which was able to travel away from the interaction point before disintegrating. More information about the whole issue can be found in <a href="http://dorigo.wordpress.com/2009/02/02/some-notes-on-the-multi-muon-analysis-part-iv/">this series of posts</a>, or by just clicking the &#8220;anomalous muons&#8221; tab in the column on the right of this text.</p>
<p>There are many things to say, but I will not say them all here now, because I am still digesting the presentation, the accompanying document produced by DZERO (not ready for public consumption yet), and the implications and subtleties involved. However, let me flash a few of the questions I am going to try and give an answer to with my readings:</p>
<ul>
<li>The paper does not address the most important question &#8211; what is DZERO&#8217;s track reconstruction efficiency as a function of track impact parameter ? They do discuss with some detail the complicated mixture of their data, which results from triggers which enforce that tracks have very small impact parameter -effectively cutting away all tracks with an impact parameter larger than 0.5cm- and a dedicated trigger which does not enforce an IP requirement; they also discuss their offline track reconstruction algorithms. But at a first sight it did not seem clear to me that they can actually reconstruct effectively tracks with impact parameters up to 2.5 cm as they claim. I would have inserted in the documents an efficiency graph for the reconstruction efficiency as a function of impact parameter, had I authored it.</li>
<li>The paper shows a distribution of the decay radius of neutral K mesons, reconstructed from their decay into pair of charged pions. From the plot, the efficiency of reconstructing those pions is <span style="color:#ff0000;">excessively smal</span>l -some three times smaller than what it is in CMS, for instance. I need to read another paper by DZERO to figure out what drives their K-zero reconstruction efficiency to be so small, and whether this is in fact due to the decrease of effectiveness with track displacement.</li>
<li>What really puzzles me, however, is the fact that <span style="color:#ff0000;">they do not see *any* excess, while we know there must be in any case a significant one: decays in flight of charged kaons and pions</span>. Why is it that CDF is riddled with those, while DZERO appears free of them ? To explain this point: charged kaons and pions yield muons, which get reconstructed as real muons with large impact parameter. If the decay occurs within the tracking volume, the track is partly reconstructed with the muon hits and partly with the kaon or pion hits. Now, while pions have a mass similar to that of muons, and thus the muon practically follows the pion trajectory faithfully, for kaons there must be a significant kink in the track trajectory. <span style="color:#ff0000;">One expects that the track reconstruction algorithm will fail to associate inner hits to a good fraction of those tracks, and the resulting muons will belong to the &#8220;loose&#8221; category, without a correspondence in the &#8220;tight&#8221; muon category which has muons containing a silicon hit in the innermost layer of the silicon detector</span>. This creates an excess of muons with large impact parameter. CDF does estimate that contribution, and it is quite large, of the order of tens of thousands of events in 743 inverse picobarns of data! Now where are those events in the DZERO dataset, then ?</li>
</ul>
<p>Of course, you should not expect that my limited intellectual capabilities and my slow reading of a paper I have had in my hands for no longer than two hours can produce foulproof arguments. So the above is just a first pass, sort of a quick and dirty evaluation. I imagine I will be able to give an answer to those puzzles myself, at least in part, with a deeper look at the documentation. But, for the time being, this is what I have to say about the DZERO analysis.</p>
<p>Or rather, I should add something. By reading the above, you might get the impression that I am only criticizing DZERO out of bitterness for the failed discovery of the century by CDF&#8230; No, it is not the case: I have always thought, and I continue to think, that the multi-muon signal by CDF is some unaccounted-for background. And I do salute with relief and interest the new effort by DZERO on this issue. I actually thank them for providing their input on this mystery. However, I still retain some scepticism with respect to the findings of their study. I hope that scepticism can be wiped off by some input &#8211; maybe some reader belonging to DZERO wants to shed some light on the issues I mentioned above ? You are most welcome to do so!</p>
<p><strong>UPDATE:</strong> <a href="http://motls.blogspot.com/2009/03/d0-debunks-lepton-jets-of-cdf.html">Lubos pitches in</a>, and guess what, he blames CDF&#8230; But Lubos the experimentalist is not better than Lubos the diplomat, if you know what I mean&#8230;</p>
<p>Other reactions will be collected below &#8211; if you have any to point to, please do so.</p>
<ul>
<li><a href="http://matpitka.blogspot.com/">Matti Pitkanen</a></li>
<li><a href="http://www.bivacco.net/marco/index.php/2009/03/18/dallaltra-parte-nessun-muone-fantasma/">Marco Dal Mastro&#8221;</a></li>
</ul>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2184/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2184/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2184/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2184/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2184/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2184/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2184/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2184/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2184/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2184/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2184&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/17/dzero-refutes-cdfs-multimuon-signal-or-does-it/feed/</wfw:commentRss>
		<slash:comments>25</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>Tevatron excludes chunk of Higgs masses!</title>
		<link>http://dorigo.wordpress.com/2009/03/13/tevatron-excludes-chunk-of-higgs-masses/</link>
		<comments>http://dorigo.wordpress.com/2009/03/13/tevatron-excludes-chunk-of-higgs-masses/#comments</comments>
		<pubDate>Fri, 13 Mar 2009 14:04:05 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2176</guid>
		<description><![CDATA[This just in &#8211; the Fermilab site has the news on the new exclusion in a range of Higgs masses. At 95% C.L., the Higgs boson cannot have a mass in the 160-170 GeV range, as shown in the graph below. The new limit is shown by the orange band.

This is the first real exclusion [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2176&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>This just in &#8211; the <a href="http://www.fnal.gov">Fermilab site</a> has the news on the new exclusion in a range of Higgs masses. At 95% C.L., the Higgs boson cannot have a mass in the 160-170 GeV range, as shown in the graph below. The new limit is shown by the orange band.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/higgsbound.jpg" alt="" /></p>
<p>This is the first real exclusion range on the Higgs boson mass from CDF and DZERO.  I will have more to say about this great new result during the weekend.</p>
<p><strong>UPDATE:</strong> maybe the most interesting thing is not the limit shown above, but the information contained in the graph shown below. It shows how the combination of CDF and DZERO searches for the Higgs bosons end up agreeing with the background-only hypothesis (black hatched curve) or the background plus signal hypothesis (red curve), as a function of the unknown value of the Higgs boson mass. The full black line seems to favor the signal plus background hypothesis, although only marginally and at just the 1-sigma level, at around 130 GeV of mass:</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/higgs09_sb.jpg" alt="" /></p>
<p>However, they say that <em>if you like sausages and if you follow laws, you should not ask how these things are made.</em> The same goes with global limits, to some extent. In this case it is not a criticism of the limit by itself, but rather of the interpretation that one might be led to give to it. In fact,<span style="color:#ff0000;"> the width of the green band should put you <em>en garde</em> against wild speculations:</span> It would be extremely suspicious if the black line did not venture outside of the green band somewhere, even in case the Higgs boson does not exist!</p>
<p>That is because the band shows the expected range of 1-sigma fluctuations -due to statistical effects, and not to systematic ones such as the real presence of a signal!- and since the black curve is extracted from the data by combining many datasets and each individual point of the line (in, say, 5-GeV intervals) has little correlation with the others,<span style="color:#ff0000;"> it is entirely appropriate for the curve to not be fully contained in the green area!</span> So, the fact that the black curve overlaps with the signal plus background hypothesis at 130 GeV really -really!- means very, very little.</p>
<p>What does mean something is that the hatched black and red curves appear separated by about one-sigma (the width of the green band surrounding the background-only black hatched curve) over a wide range of Higgs masses. This says that the two Tevatron experiments have by now reached a sensitivity of about 1-sigma to the signal with the data they have analyzed so far. Beware: they are already sitting on about twice as much data (most analyses rely on about 2.5/fb of collisions, but the Tevatron has already delivered to the experiments over 5/fb). So they expect new results, significantly improved, by this summer.</p>
<p>It does seem that at last, the game of Higgs hunting is starting to get exciting again, after a hiatus of about 7 years following the tentative signal seen by the LEP II experiments!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2176/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2176/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2176/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2176/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2176/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2176/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2176/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2176/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2176/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2176/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2176&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/13/tevatron-excludes-chunk-of-higgs-masses/feed/</wfw:commentRss>
		<slash:comments>43</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/higgsbound.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/higgs09_sb.jpg" medium="image" />
	</item>
		<item>
		<title>CDF discovers a new hadron!</title>
		<link>http://dorigo.wordpress.com/2009/03/13/cdf-discovers-a-new-hadron/</link>
		<comments>http://dorigo.wordpress.com/2009/03/13/cdf-discovers-a-new-hadron/#comments</comments>
		<pubDate>Fri, 13 Mar 2009 07:55:51 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[discoveries]]></category>
		<category><![CDATA[QCD]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2142</guid>
		<description><![CDATA[This morning CDF released the results of a search for narrow resonances produced in B meson decays, and in turn decaying into a pair of vector mesons: namely, . This Y state is a new particle whose exact composition is as of yet unknown, except that CDF has measured its mass (4144 MeV) and established [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2142&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>This morning CDF <a href="http://arxiv.org/abs/0903.2229">released the results</a> of a search for narrow resonances produced in B meson decays, and in turn decaying into a pair of vector mesons: namely, <img src='http://l.wordpress.com/latex.php?latex=Y+%5Cto+J%2F%5Cpsi+%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Y \to J/\psi \phi' title='Y \to J/\psi \phi' class='latex' />. This Y state is a new particle whose exact composition is as of yet unknown, except that CDF has measured its mass (4144 MeV) and established that its decay appears to be mediated by strong interactions, given that the natural width of the state is in the range of a few MeV. I describe succintly the analysis below, but first let me make a few points on the relevance of area of investigation.</p>
<p>Heavy meson spectroscopy appears to be a really entertaining research field these days. While all eyes are pointed at the searches for the Higgs boson and supersymmetric particles, if not at even more exotic high-mass objects, and while careers are made and unmade on those uneventful searches, it is elsewhere that action develops. Just think about it: the <img src='http://l.wordpress.com/latex.php?latex=%5CXi_b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\Xi_b' title='\Xi_b' class='latex' /> baryon, the <img src='http://l.wordpress.com/latex.php?latex=%5COmega_b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\Omega_b' title='\Omega_b' class='latex' />, those mysterious X and Y states which are still unknown in their quark composition. Such discoveries tell the tale of a very prolific research field: one where there is really a lot to understand.</p>
<p>Low-energy QCD  is still poorly known and not easily calculable. In frontier High-Energy Physics we bypassed the problem for the sake of studying high-energy phenomena by tuning our simulations such that their output well resembles the result of low-energy QCD processes in all cases where we need them -such as the details of parton fragmentation, or jet production, or transverse momentum effects in the production of massive bodies. However, we have not learnt much with our parametrizations:  those describe well what we already know, but they do not even come close to guessing whatever we do not know. Our understanding of low-energy QCD is starting to be a limiting factor in cosmological studies, such as in baryogenesis predictions. So by all means, let us pursue low-energy QCD in all the dirty corners of our produced datasets at hadron colliders!</p>
<p>CDF is actively pursuing this task. The outstanding spectroscopic capabilities of the detector, combined with the huge size of the dataset collected since 2002, allow searches for decays in the one-in-a-million range of branching ratios. The new discovery I am discussing today has indeed been made possible by pushing to the limit our search range.</p>
<p>The full decay chain which has been observed is the following: <img src='http://l.wordpress.com/latex.php?latex=B%5E%2B+%5Cto+Y+K%5E%2B+%5Cto+J%2F%5Cpsi+%5Cphi+K%5E%2B+%5Cto+%5Cmu%5E%2B+%5Cmu%5E-+K%5E%2B+K%5E-+K%5E%2B&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='B^+ \to Y K^+ \to J/\psi \phi K^+ \to \mu^+ \mu^- K^+ K^- K^+' title='B^+ \to Y K^+ \to J/\psi \phi K^+ \to \mu^+ \mu^- K^+ K^- K^+' class='latex' />. That <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi' title='J/\psi' class='latex' /> mesons decay to muon pairs is not a surprise, as is the decay to two charged kaons of the <img src='http://l.wordpress.com/latex.php?latex=%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\phi' title='\phi' class='latex' /> vector meson. Also the original decay of the B hadron into the <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi+%5Cphi+K&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi \phi K' title='J/\psi \phi K' class='latex' /> final state is not new: it had been in fact observed previously. What had not been realized yet, because of the insufficient statistics and mass resolution, is that the <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi' title='J/\psi' class='latex' /> and <img src='http://l.wordpress.com/latex.php?latex=%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\phi' title='\phi' class='latex' /> mesons produced in that reaction often &#8220;resonate&#8221; at a very definite mass value, indicating that in those instances the <img src='http://l.wordpress.com/latex.php?latex=B+%5Cto+J%2F%5Cpsi+%5Cphi+K&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='B \to J/\psi \phi K' title='B \to J/\psi \phi K' class='latex' /> decay actually takes place in two steps as the chain of two two-body decays: <img src='http://l.wordpress.com/latex.php?latex=B+%5Cto+Y+K&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='B \to Y K' title='B \to Y K' class='latex' /> and <img src='http://l.wordpress.com/latex.php?latex=Y+%5Cto+J%2F%5Cpsi+%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Y \to J/\psi \phi' title='Y \to J/\psi \phi' class='latex' />.</p>
<p>The new analysis by CDF is a pleasure to examine, because the already excellent momentum resolution of the charged particle tracking system gets boosted when constraints are placed on the combined mass of multi-body systems. Take the B meson, reconstructed with two muons and three charged tracks, each assumed to be a kaon: if you did not know that the muon pair comes from a <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi' title='J/\psi' class='latex' /> nor that two of the kaons come from a <img src='http://l.wordpress.com/latex.php?latex=%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\phi' title='\phi' class='latex' />, the mass resolution of the system would be in the few tens of MeV range. Instead, by forcing the momenta of the two muons to be consistent with the World average mass of the <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi' title='J/\psi' class='latex' />, <img src='http://l.wordpress.com/latex.php?latex=M_%7BJ%2F%5Cpsi%7D%3D3096.916+%5Cpm+0.011+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_{J/\psi}=3096.916 \pm 0.011 MeV' title='M_{J/\psi}=3096.916 \pm 0.011 MeV' class='latex' /> , and by imposing that the two kaons make exactly the extremely well-known <img src='http://l.wordpress.com/latex.php?latex=%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\phi' title='\phi' class='latex' /> mass (<img src='http://l.wordpress.com/latex.php?latex=M_%5Cphi%3D1019.455+%5Cpm+0.020+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_\phi=1019.455 \pm 0.020 MeV' title='M_\phi=1019.455 \pm 0.020 MeV' class='latex' />), much of the uncertainty on the daughter particle momenta disappears, and the B meson becomes an extremely narrow signal: its mass resolution is just 5.9 MeV, a per-mille measurement event-by-event!</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/Ymasses.jpg" alt="" width="460" /></p>
<p>The selection of signal events requires several cleanup cuts, including mass window cuts around the J/Psi and phi masses, a decay length of the reconstructed B+ meson longer than 500 microns, and a cut on the log-likelihood ratio fed with dE/dx and time-of-flight information capable of discriminating kaon tracks from other hadrons. After those cuts, the B+ signal really stands above the flat background. There is a total of 78+-10 events in the sample after these cuts, and this is the largest sample of such decays ever isolated. It is shown above (left), together with the corresponding distribution in the <img src='http://l.wordpress.com/latex.php?latex=%5Cphi+%5Cto+KK&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\phi \to KK' title='\phi \to KK' class='latex' /> candidate mass (right).</p>
<p><img class="alignright" src="http://www.pd.infn.it/~dorigo/Ydalitz.jpg" alt="" />A Dalitz plot of the reconstructed decay candidates is shown in the figure on the right. A Dalitz plot is a scatterplot of the squared invariant mass of a subset of the particles emitted in the decay, versus the squared invariant mass of another subset. If the decay proceeds via the creation of an intermediate state, one may observe a horizontal or vertical cluster of events. Judge by yourself: do the points appear to spread evenly in the allowed phase space of the B+ decays ?</p>
<p>The answer is no: a significant structure is seen corresponding to a definite mass of the <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi+%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi \phi' title='J/\psi \phi' class='latex' /> system. A histogram of the difference between the reconstructed mass of the <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi+%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi \phi' title='J/\psi \phi' class='latex' /> system and the <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi' title='J/\psi' class='latex' /> mass is shown in the plot below: a near-threshold structure appears at just above 1 GeV energy. An unbinned fit to a relativistic Breit-Wigner signal shape on top of the expected background shape shows a signal at a mass difference of <img src='http://l.wordpress.com/latex.php?latex=%5CDelta+M%3D1046.3+%5Cpm+2.9+MeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\Delta M=1046.3 \pm 2.9 MeV' title='\Delta M=1046.3 \pm 2.9 MeV' class='latex' />, with a width of 11.7+-5.7 MeV.</p>
<p><img class="alignleft" src="http://www.pd.infn.it/~dorigo/Ypeak.jpg" alt="" /> The significance of the signal is, after taking account of trial factors, equal to 3.8 standard deviations. For the non-zero width hypothesis, the significance is of 3.4 standard deviations, implying that the newfound structure has strong decay. The mass of the new state is thus of 4143+-2.9 MeV.</p>
<p>The new state is above the threshold for decay to pair of charmed hadrons. The decay of the state appears to occur to a pair of vector mesons, <img src='http://l.wordpress.com/latex.php?latex=J%2F%5Cpsi+%5Cphi&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='J/\psi \phi' title='J/\psi \phi' class='latex' />, in close similarity to a previous state found at 3930 MeV, the Y(3930), which also decays to two vector mesons in <img src='http://l.wordpress.com/latex.php?latex=Y+%5Cto+J%2F%5Cpsi+%5Comega&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Y \to J/\psi \omega' title='Y \to J/\psi \omega' class='latex' />. Therefore, the new state can be also called a Y(4140).</p>
<p>Although the significance of this new signal has not reached the coveted threshold of 5 standard deviations, there are few doubts about its nature. Being a die-hard sceptic, I did doubt about the reality of the signal shown above for a while when I first saw it, but I must admit that the analysis was really done with a lot of care. Besides, CDF now has tens of thousands of fully reconstructed B meson decays available, with which it is possible to study and understand even the most insignificant nuances to every effect, including reconstruction problems, fit method, track characteristics, kinematical biases, you name it. So I am bound to congratulate with the authors of this nice new analysis, which shows once more how the CDF experiment is producing star new results not just in the high-energy frontier, but as well as in low-energy spectroscopy. Well done, CDF!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2142/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2142/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2142/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2142/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2142/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2142/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2142/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2142/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2142/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2142/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2142&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/13/cdf-discovers-a-new-hadron/feed/</wfw:commentRss>
		<slash:comments>25</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/Ymasses.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/Ydalitz.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/Ypeak.jpg" medium="image" />
	</item>
		<item>
		<title>Live video streaming of single top observation NOW</title>
		<link>http://dorigo.wordpress.com/2009/03/10/live-video-streaming-of-single-top-observation-now/</link>
		<comments>http://dorigo.wordpress.com/2009/03/10/live-video-streaming-of-single-top-observation-now/#comments</comments>
		<pubDate>Tue, 10 Mar 2009 19:32:34 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top quark]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2146</guid>
		<description><![CDATA[You can follow it at this link.
       <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2146&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>You can follow it <a href="http://www-visualmedia.fnal.gov/VMS_Site_2/index.shtml">at this link</a>.</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2146/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2146/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2146/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2146/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2146/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2146/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2146/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2146/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2146/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2146/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2146&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/10/live-video-streaming-of-single-top-observation-now/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>Who discovered single top production ?</title>
		<link>http://dorigo.wordpress.com/2009/03/05/who-discovered-single-top-production/</link>
		<comments>http://dorigo.wordpress.com/2009/03/05/who-discovered-single-top-production/#comments</comments>
		<pubDate>Thu, 05 Mar 2009 15:17:51 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top quark]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2123</guid>
		<description><![CDATA[Both CDF and DZERO have announced yesterday the first observation of electroweak production of single top quarks in proton-antiproton collisions. Both papers (this one from CDF, and this one from DZERO) claim theirs is the first observation of the long sought-after subatomic reaction. Who is right ? Who has more merit in this advancement in [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2123&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Both CDF and DZERO have announced yesterday the first observation of electroweak production of single top quarks in proton-antiproton collisions. Both papers (<a href="http://www-cdf.fnal.gov/physics/new/top/stprl09.pdf">this one</a> from CDF, and <a href="http://arxiv.org/PS_cache/arxiv/pdf/0903/0903.0850v1.pdf">this one</a> from DZERO) claim theirs is the first observation of the long sought-after subatomic reaction. <span style="color:#0000ff;"><strong>Who is right ? </strong>Who has more merit in this advancement in human knowledge of fundamental interactions ? Whose analysis is more credible ? Which of the two results has fewer blemishes ?</span></p>
<p>To me, it is always a matter of which one is the most relevant question. And to me, the most relevant question is, <span style="color:#ff0000;"><strong>Who cares who did it ?</strong> .<span style="color:#000000;">.. with the easy-to-guess answer: <strong>not me</strong>. As I have had other occasions to say, I am for the advancement of Science, much less for the advancement of scientific careers, leave alone to which experiments those careers belong.</span><br />
</span></p>
<p><img class="alignright" src="http://www.pd.infn.it/~dorigo/singletopobs_diags.jpg" alt="" width="373" height="140" />The top quark is interesting, but so far the Tevatron experiments had only studied it when produced in pairs with its antiparticle, through strong interactions. Electroweak production of the top quark is also possible in proton-antiproton collisions, at half the rate. It is one of those rare instances when the electroweak force competes with the strong one, and it is due to the large mass of the top quark: producing two is much more demanding than producing only one, due to the limited energy budget of the collisions. The reactions capable of producing a single top quark are described by the diagrams shown above. In a), a b-quark from one of the projectiles becomes a top by intervention of a weak vector boson; in b), a gluon &#8220;fuses&#8221; with a W boson and a top quark is created; in c), a W boson is produced off-mass-shell, and it possesses enough energy to decay into a top-bottom pair.</p>
<p>Since 1995, when CDF and DZERO published jointly the observation of the top quark, nobody has ever doubted that electroweak processes would produce single tops as well. Not even one article, to my knowledge, tried to speculate that the top might be so special to have no weak couplings. The very few early attempts at casting doubt on the real nature of what the Tevatron experiments were producing died quickly as statistics improved and the characterization of the newfound quark was furthered.<span style="color:#ff0000;"> So what is the fuss</span> about finding out that the reaction resulting from the Feynman diagrams shown above can indeed be directly observed ?</p>
<p>There are different facets in a thorough answer to  the above question. <span style="color:#0000ff;">First of all,</span> competition between CDF and DZERO: each collaboration badly wanted to get there first, especially since this was correctly predicted from the outset to be a tough nut to crack. <span style="color:#0000ff;">Second</span>, because seeing single top production implies having direct access to one element of the Cabibbo-Kobayashi-Maskawa mixing matrix, the element <img src='http://l.wordpress.com/latex.php?latex=V_%7Btb%7D&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='V_{tb}' title='V_{tb}' class='latex' />, which is after all a fundamental parameter in the standard model (well, to be precise it is a <em>function</em> of some of the latter, namely of the CKM matrix parameters, but let&#8217;s not split hairs here). <span style="color:#0000ff;">Third,</span> you cannot really see a low-mass Higgs at the Tevatron if you did not measure single top production first, because single top is a background in Higgs boson searches, and one cannot really discover something by assuming something else is there, if one has not proven that beforehand.</p>
<p>So, single top observation is important after all. I am a member of the CDF collaboration, and I am really proud I belong to it, so my judgement on the whole issue might be biased. But if I have to answer the question that gave the title to this post, I will first give you a very short summary of  the results of the two analyses,  deferring to a better day a more detailed discussion. This will allow me to drive home a few points.</p>
<p>The two analyses: a face-to-face summary</p>
<ul>
<li>Significance: both experiments claim that the signal they observe has a statistical significance of 5.0 standard deviations.</li>
</ul>
<ol>
<li>CDF uses 3.2 inverse femtobarns, and finds a 5.0-sigma-significance signal of single top production. The sensitivity of the analysis is better measured by the expected significance, which is quoted at <span style="color:#ff0000;">5.9-sigma</span>.</li>
<li>DZERO uses 2.4 inverse femtobarns, and finds a 5.0-sigma-significance of single top production. The sensitivity of the DZERO analysis is quoted at <span style="color:#ff0000;">4.5-sigma</span>.</li>
</ol>
<ul>
<li>Cross-section: both experiments measure a cross section in agreement with standard model expectations.</li>
</ul>
<ol>
<li>CDF measures <img src='http://l.wordpress.com/latex.php?latex=%5Csigma+%3D+2.3%5E%7B%2B0.6%7D%7B-0.5%7D+pb&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\sigma = 2.3^{+0.6}{-0.5} pb' title='\sigma = 2.3^{+0.6}{-0.5} pb' class='latex' />, a relative uncertainty of about <span style="color:#ff0000;">24%.</span></li>
<li>DZERO measures <img src='http://l.wordpress.com/latex.php?latex=%5Csigma+%3D+3.9+%5Cpm+0.9+pb&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\sigma = 3.9 \pm 0.9 pb' title='\sigma = 3.9 \pm 0.9 pb' class='latex' />, a relative uncertainty of about <span style="color:#ff0000;">23%</span>.</li>
</ol>
<ul>
<li>Measurements of the CKM matrix element: both experiments quote a direct determination of that quantity, which is very close to 1.0 in the SM, but cannot exceed unity.</li>
</ul>
<ol>
<li>CDF finds <img src='http://l.wordpress.com/latex.php?latex=%7CV_%7Btb%7D%7C%3D0.91+%5Cpm+0.11&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='|V_{tb}|=0.91 \pm 0.11' title='|V_{tb}|=0.91 \pm 0.11' class='latex' />, a <span style="color:#ff0000;">12%</span> accuracy.</li>
<li>DZERO finds <img src='http://l.wordpress.com/latex.php?latex=%7CV_%7Btb%7D%7C%3D1.07+%5Cpm+0.12&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='|V_{tb}|=1.07 \pm 0.12' title='|V_{tb}|=1.07 \pm 0.12' class='latex' />, a <span style="color:#ff0000;">11%</span> accuracy.</li>
</ol>
<ul>
<li>Data distributions: both experiments have a super-discriminant which combines the information from different searches. This is a graphical display of the power of the analysis, and should be examined with care.</li>
</ul>
<p>1. CDF in its paper shows the distribution below, as well as the five inputs that were used to obtain it. The distribution shows the single-top contribution in red, stacked over the concurring backgrounds. At high values of the discriminant, the single top signal does stick out, and the black points -the data- follow the sum of all processes nicely.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/singletopobs_cdf.jpg" alt="" width="460" /></p>
<p>2.DZERO in its paper has only the distribution shown below. I was underwhelmed when I saw it. Again, backgrounds are stacked one on top of the other, the top distribution is the one from single top (this time shown in blue), and the data is shown by black dots. It does not look like the data prefer the hypothesis of backgrounds+single top over the background-only one all that much!</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/singletopobs_d0.jpg" alt="" width="460" /></p>
<p>Maybe I am too partisan to really make a credible point here, and since I did not follow in detail the development of these analyses -from their first publications as evidence for single top, to updates, until yesterday&#8217;s papers- I may very well be proven wrong; however, by looking at the two plots above, and by knowing that they both appear to provide a 5.0-sigma significance, <span style="color:#0000ff;">I am drawn to the conclusion that DZERO believes their background shapes and normalization much better than CDF does</span>!</p>
<p>Now, believing something is a good thing in almost all human activities except Science. And if two scientific collaborations have a very different way of looking at how well their backgrounds are modeled by Monte Carlo simulations (which, at least as far as the generation of subatomic processes is concerned, are -or can be- the same), which one is to praise more: the one which believes the simulations more to extract their signal, or the one which relies less on them?</p>
<p>The above question is rethorical, and you should have already agreed that you value more a result which is less based on simulations. So let us look into this issue a bit further. <span style="color:#ff0000;"><span style="color:#0000ff;">CDF bases its result on a total sample of 4780 events, where the total uncertainty is estimated at +-533 events. DZERO bases its own on a sample of 4651 events, with a total uncertainty estimated at +-234 events! </span>What drives such a large difference in the precision of these predictions ?</span></p>
<p><span style="color:#ff0000;"><span style="color:#000000;">The culprit is one of the backgrounds, the production of W bosons in association with heavy flavor quarks &#8211; an annoying process, which enters all selection of top quarks and Higgs bosons at the Tevatron. CDF has it at 1855 events, with an uncertainty of 486 -or 26.2%; it is shown in green in the CDF plot above. DZERO has it at 2646 events, with an uncertainty of 173, or 6.5%; it is also shown in green in the DZERO plot.  Do not be distracted by the different size of the contribution of W+heavy flavor in the two datasets: different selection strategies drive the numbers to differ, and besides, it is rather the total number of events of the two analyses which is similar by pure chance. The point here is the uncertainty.</span></span></p>
<p><span style="color:#ff0000;"><span style="color:#000000;">Luckily, the DZERO analysis does not appear to rely too much on the background normalization -this is not a simple counting experiment, where the better you know the size of expected backgrounds, the smaller your uncertainty on the signal; rather, <span style="color:#ff0000;">the<em> shapes </em>of backgrounds are important</span>, and the graphs above show that the data appears indeed well-described by the discriminant shape. And of course, background shapes are checked in control samples, so both experiments have many tools to ensure that the different contributions are well understood. However, the issue remains: how much do the different estimates of the W plus heavy flavor uncertainty impacts the significance of the measurements ? The DZERO paper mentions that one of their largest uncertainties arises from the modeling of the heavy flavor composition of W+jet events, but it does not provide further details.<br />
</span></span></p>
<p><span style="color:#ff0000;"><span style="color:#000000;">I would be happy to receive an informed answer in the comments thread about the points I mention above&#8230;<br />
</span></span></p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2123/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2123/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2123/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2123/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2123/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2123/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2123/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2123/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2123/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2123/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2123&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/05/who-discovered-single-top-production/feed/</wfw:commentRss>
		<slash:comments>39</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/singletopobs_diags.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/singletopobs_cdf.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/singletopobs_d0.jpg" medium="image" />
	</item>
		<item>
		<title>First observation of single top production from CDF!!!</title>
		<link>http://dorigo.wordpress.com/2009/03/05/first-observation-of-single-top-production-from-cdf/</link>
		<comments>http://dorigo.wordpress.com/2009/03/05/first-observation-of-single-top-production-from-cdf/#comments</comments>
		<pubDate>Thu, 05 Mar 2009 07:31:33 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top quark]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2115</guid>
		<description><![CDATA[The paper, submitted to PRL yesterday evening, is here.
I will discuss the details later today&#8230;
UPDATE: a reader points out that the above link was broken. Now fixed.
       <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2115&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>The paper, submitted to PRL yesterday evening, is <a href="http://www-cdf.fnal.gov/physics/new/top/stprl09.pdf">here</a>.<br />
I will discuss the details later today&#8230;</p>
<p><strong>UPDATE:</strong> a reader points out that the above link was broken. Now fixed.</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2115/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2115/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2115/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2115/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2115/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2115/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2115/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2115/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2115/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2115/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2115&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/05/first-observation-of-single-top-production-from-cdf/feed/</wfw:commentRss>
		<slash:comments>15</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>Higgs decays to photon pairs!</title>
		<link>http://dorigo.wordpress.com/2009/03/04/higgs-decays-to-photon-pairs/</link>
		<comments>http://dorigo.wordpress.com/2009/03/04/higgs-decays-to-photon-pairs/#comments</comments>
		<pubDate>Wed, 04 Mar 2009 11:44:16 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[DZERO]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LHC]]></category>
		<category><![CDATA[photons]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2107</guid>
		<description><![CDATA[It was with great pleasure that I found yesterday, in the public page of the DZERO analyses, a report on their new search for Higgs boson decays to photon pairs. On that quite rare decay process -along with another not trivial decay, the  reaction- the LHC experiments base their hopes to see the Higgs [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2107&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>It was with great pleasure that I found yesterday, in the <a href="http://www-d0.fnal.gov/Run2Physics/WWW/results.htm">public page of the DZERO analyses, a <a href="http://www-d0.fnal.gov/Run2Physics/WWW/results/prelim/HIGGS/H66/">report</a> on their new search for Higgs boson decays to photon pairs. On that quite rare decay process -along with another not trivial decay, the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+%5Ctau+%5Ctau&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to \tau \tau' title='H \to \tau \tau' class='latex' /> reaction- the LHC experiments base their hopes to see the Higgs boson if that particle has a mass close to the LEP II upper bound, i.e. not far from 115 GeV. And this is the first high-statistics search for the SM Higgs in that final state to obtain results that are competitive with the more standard searches!</p>
<p>My delight was increased when I saw that results of the DZERO search are based on a data sample corresponding to a whooping <span style="color:#ff0000;">4.2 inverse-femtobarns of integrated luminosity</span>. This is the largest set of hadron-collider data ever used for an analysis. 4.2 inverse femtobarns correspond to about <span style="color:#ff0000;">three-hundred <em>trillion</em> collisions</span>, sorted out by DZERO. Of course, both DZERO and CDF have so far collected more than that statistics: almost five inverse femtobarns. However, it always takes some time before calibration, reconstruction, and production of the newest datasets is performed&#8230; DZERO is catching up nicely with the accumulated statistics, it appears.</p>
<p>The most interesting few tens of billions or so of those events have been fully reconstructed by the software algorithms, identifying charged tracks, jets, electrons, muons, and photons. Yes, <span style="color:#0000ff;">photons</span>: quanta of light, only very energetic ones: gamma rays.</p>
<p>When photons have an energy exceeding a GeV or so (i.e. one corresponding to a proton mass or above), they can be counted and measured individually by the electromagnetic calorimeter. One must look for very localized energy deposits which cannot be spatially correlated with a charged track: something hits the calorimeter after crossing the inner tracker, but no signal is found there, implying that the object was electrically neutral. The shape of the energy deposition then confirms that one is dealing with a single photon, and not -for instance- a neutron, or a pair of photons traveling close to each other. Let me expand on this for a moment.</p>
<p><strong>Background sources of photon signals</strong></p>
<p>In general, every proton-antiproton collision yield dozens, or even hundreds of energetic photons. This is not surprising, as there are multiple significant sources of GeV-energy gamma rays to consider.</p>
<ol>
<li><img class="alignright" src="http://www.pd.infn.it/~dorigo/bremsstrahlung.gif" alt="" width="200" />Electrons, as well as in principle any other electrically charged particle emitted in the collision, have the right to produce photons by the process called <span style="color:#ff0000;">bremsstrahlung</span>: by passing close to the electric field generated by a heavy nucleus, the particle emits electromagnetic radiation, thus losing a part of its energy. Note that this is a process which cannot happen in vacuum, since there are no target nuclei there to supply the electric field with which the charged particle interacts (one can have bremsstrahlung also in the presence of neutral particles, in principle, since what matters is the capability of the target to absorb a part of the colliding body&#8217;s momentum; but in that case, one needs a more complicated scattering process, so let us forget about it). For particles heavier than the electron, the process is suppressed up to the very highest energy (where particle masses are irrelevant with respect to their momenta), and is only worth mentioning for muons and pions in heavy materials.</li>
<li>By far the most important process for photon creation at a collider is the <span style="color:#ff0000;">decay of neutral hadrons</span>. A high-energy collision at the Tevatron easily yields a dozen of neutral pions, and these particles decay more than 99% of the time into pairs of photons, <img src='http://l.wordpress.com/latex.php?latex=%5Cpi%5E%5Ccirc+%5Cto+%5Cgamma+%5Cgamma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\pi^\circ \to \gamma \gamma' title='\pi^\circ \to \gamma \gamma' class='latex' />. Of course, these photons would only have an energy equal to half the neutral pion mass -0.07 GeV- if the neutral pions were at rest; it is only through the large momentum of the parent that the photons may be energetic enough to be detected in the calorimeter.</li>
<li>A similar fate to that of neutral pions awaits other neutral hadrons heavier than the <img src='http://l.wordpress.com/latex.php?latex=%5Cpi%5E%5Ccirc&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\pi^\circ' title='\pi^\circ' class='latex' />: most notably the particle called eta, in the decay <img src='http://l.wordpress.com/latex.php?latex=%5Ceta+%5Cto+%5Cgamma+%5Cgamma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\eta \to \gamma \gamma' title='\eta \to \gamma \gamma' class='latex' />. The eta has a mass four times larger than that of the neutral pion, and is less frequently produced.</li>
<li>And other hadrons may produce photons in <span style="color:#ff0000;">de-excitation processes</span>, albeit not in pairs: excited hadrons often decay radiatively into their lower-mass brothers, and the radiated photon may display a significant energy, again critically depending on the parent&#8217;s speed in the laboratory.</li>
</ol>
<p>All in all, that&#8217;s quite a handful of photons our detectors are showered with on an event-by-event basis! How the hell can DZERO sort out then, amidst over three hundred trillion collisions, the maybe five or ten which saw the decay of a Higgs to two photons ?</p>
<p><strong>And the Higgs signal amounts to&#8230;<br />
</strong></p>
<p><span style="color:#0000ff;">Five to ten events</span>. Yes, we are talking of a tiny signal here. To eyeball how many standard model Higgs boson decays to photon pairs we may expect in a sample of 4.2 inverse femtobarns, we make some approximations. First of all, we take a 115 GeV Higgs for a reference: that is the Higgs mass where the analysis should be most sensitive, if we accept that the Higgs cannot be much lighter than that: for heavier higgses, their number will decrease, because the heavier a particle is, the less frequently it is produced.</p>
<p>The cross-section for the direct-production process <img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+H+%2B+X&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to H + X' title='p \bar p \to H + X' class='latex' /> (where with X we denote our unwillingness to specify whatever else may be produced together with the Higgs) is, at the Tevatron collision energy of 1.96 TeV, of the order of one picobarn. I am here purposedly avoiding to fetch a plot of the xs vs mass to give you the exact number: it is in that ballpark, and that is enough.</p>
<p>The other input we need is the <em>branching ratio </em>of H decay to two photons. This is the <span style="color:#ff0000;">fraction of disintegrations </span>yielding the final state that DZERO has been looking for. It depends on the detailed properties of the Higgs particle, which likes to couple to particles depending on the mass of the latter. <span style="color:#0000ff;">The larger a particle&#8217;s mass, the stronger its coupling to the Higgs</span>, and the more frequent the H decay into a pair of those: the branching fraction depends on the squared mass of the particle, but since the sum of all branching ratios is one -if we say the Higgs decays, then there is a 100% chance of its decaying into <em>something</em>, no less and no more!- <span style="color:#ff0000;">any branching fraction depends on ALL other particle masses!!!</span></p>
<p><img class="alignright" src="http://www.pd.infn.it/~dorigo/hggdecay.gif" alt="" width="299" height="170" />&#8220;Wait a minute,&#8221; I would like to hear you say now, &#8220;the photon is massless! How can the Higgs couple to it?!&#8221;. Right. H does not couple directly to photons, but it can nevertheless decay into them via a virtual loop of electrically charged particles. <em>Just as happens when your US plug won&#8217;t fit into an european AC outlet! You do not despair, and insert an adaptor: something endowed with the right holes on one side and pins on the other.</em> Much in the same way, a virtual loop of top quarks, for instance, will do a good job: the top has a large mass -so it couples aplenty to the Higgs- and it has an electric charge, so it is capable of emitting photons. The three dominant Feynman diagrams for the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+%5Cgamma+%5Cgamma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to \gamma \gamma' title='H \to \gamma \gamma' class='latex' /> decay are shown above: the first two of them involve a loop of W bosons, the third a loop of top quarks.</p>
<p>So, how much is the branching ratio to two photons in the end ? It is a complicated calculus, but the result is roughly <span style="color:#ff0000;">one thousandth</span>. One in a thousand low-mass Higgses will disintegrate into energetic light: two angry gamma rays, each roughly carrying the energy of a 2 milligram mosquito launched at the whooping speed of four inches per second toward your buttocks.</p>
<p>Now we have all the ingredients for our computation of the number of signal events we may be looking at, amidst the trillions produced. The master formula is just</p>
<p><img src='http://l.wordpress.com/latex.php?latex=N+%3D+%5Csigma+L+B&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='N = \sigma L B' title='N = \sigma L B' class='latex' /></p>
<p>where <img src='http://l.wordpress.com/latex.php?latex=N&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='N' title='N' class='latex' /> is the number of decays of the kind we want, <img src='http://l.wordpress.com/latex.php?latex=%5Csigma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\sigma' title='\sigma' class='latex' /> is the production cross section for Higgs at the Tevatron, <img src='http://l.wordpress.com/latex.php?latex=L&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='L' title='L' class='latex' /> is the integrated luminosity on which we base our search, and B is the branching ratio of the decay we study.</p>
<p>With <img src='http://l.wordpress.com/latex.php?latex=%5Csigma+%3D+1pb&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\sigma = 1pb' title='\sigma = 1pb' class='latex' />, <img src='http://l.wordpress.com/latex.php?latex=L%3D4.2+fb%5E%7B-1%7D+%3D+4200+pb%5E%7B-1%7D&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='L=4.2 fb^{-1} = 4200 pb^{-1}' title='L=4.2 fb^{-1} = 4200 pb^{-1}' class='latex' />, and <img src='http://l.wordpress.com/latex.php?latex=B%3D0.001&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='B=0.001' title='B=0.001' class='latex' />, the result is, guess what, 4.2 events. <span style="color:#ff0000;">4.2 in three hundred trillions</span>. A needle in the haystack is a kids&#8217; game in comparison!</p>
<p><strong>The DZERO analysis</strong></p>
<p>I will not spend much of my and your time discussing the details of the DZERO analysis here, primarily because this post is already rather long, but also because the analysis is pretty straightforward to describe at an elementary level: one selects events with two photons of suitable energy, computes their combined invariant mass, and compares the expectation for Higgs decays -a roughly bell-shaped curve centered at the Higgs mass and with a width of ten GeV or so- with the expected backgrounds from all the processes capable of yielding pairs of energetic photons, plus all those yielding fake photons. [Yes, fake photons: of course the identification of gamma rays is not perfect -one may have not detected a charged track pointing at the calorimeter energy deposit, for instance.] Then, a fit of the mass distribution extracts an upper limit on the number of signal events that may be hiding there. From the upper limit on the signal size, an upper limit is obtained on the signal cross-section.</p>
<p>Ok, the above was a bit too quick. Let me be slightly more analytic. The data sample is collected by an online trigger requiring two isolated electromagnetic deposits in the calorimeter. Offline, the selection requires that both photon candidates have a transverse energy exceeding 25 GeV, and that they be isolated from other calorimetric activity -a requirement which removes fake photons due to hadronic jets.</p>
<p>Further, there must be no charged tracks pointing close to the deposit, and a neural-network classifier is used to discriminate real photons from backgrounds using the shape of the energy deposition and other photon quality variables. The NN output is shown in the figure below: real photons (described by the red histogram) cluster on the right. A cut on the data (black points) of a NN output larger than 0.1 accepts almost all signal and removes 50% of the backgrounds (the hatched blue histogram). One important detail: the shape of the NN output for real high-energy photons is modeled by Monte Carlo simulations, but is found in good agreement with that of real photons in radiative Z boson decay processes, <img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+l%5E%2B+l%5E-+%5Cgamma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to l^+ l^- \gamma' title='p \bar p \to l^+ l^- \gamma' class='latex' />. In those processes, the detected photon is 100% pure!</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/hggdzerogammann.jpeg" alt="" width="460" /></p>
<p>After the selection, surviving backgrounds are due to three main processes: real photon pairs produced by quark-antiquark interactions, compton-like gamma-jet events where the jet is mistaken for a photon, and Drell-Yan processes yielding two electrons, both of which are mistaken for photons. You can see the relative importance of the three sources in the graph below, which shows the diphoton invariant mass distribution for the data (black dots) compared to the sum of backgrounds. Real photons are in green, compton-like gamma-jet events are in blue, and the Drell-Yan contribution is in yellow.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/hggdzerobgrs.jpeg" alt="" width="460" /></p>
<p>The mass distribution has a very smooth exponential shape, and to search for Higgs events DZERO fits the spectrum with an exponential, obliterating a signal window where Higgs decays may contribute. The fit is then extrapolated into the signal window, and a comparison with the data found there provides the means for a measurement; different signal windows are assumed to search for different Higgs masses. Below are shown four different hypotheses for the Higgs mass, ranging from 120 to 150 GeV in 10-GeV intervals. The expected signal distribution, shown in purple, is multiplied by a factor x50 in the plots, for display purposes.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/hggdzeromasses42.jpg" alt="" width="460" /></p>
<p>From the fits, a 95% upper limit on the Higgs boson production cross section is extracted by standard procedures. As by now commonplace, the cross-section limit is displayed by dividing it by the expected standard model Higgs cross section, to show how far one is from excluding the SM-produced Higgs at any mass value. The graph is shown below: readers of this blog may by now recognize at first sight the green 1-sigma and yellow 2-sigma bands showing the expected range of limits that the search was predicted to set. The actual limit is shown in black.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/hggdzerolim42fb.jpeg" alt="" width="460" /></p>
<p>One notices that while this search is not sensitive to the Higgs boson yet, it is not so far from it any more! The LHC experiments will have a large advantage with respect to DZERO (and CDF) in this particular business, since there the Higgs production cross-section is significantly larger. Backgrounds are also larger, however, so a detailed understanding of the detectors will be required before such a search is carried out with success at the LHC. For the time being, I congratulate with my DZERO colleagues for pulling off this nice new result!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2107/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2107/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2107/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2107/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2107/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2107/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2107/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2107/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2107/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2107/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2107&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/04/higgs-decays-to-photon-pairs/feed/</wfw:commentRss>
		<slash:comments>19</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/bremsstrahlung.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/hggdecay.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/hggdzerogammann.jpeg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/hggdzerobgrs.jpeg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/hggdzeromasses42.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/hggdzerolim42fb.jpeg" medium="image" />
	</item>
		<item>
		<title>Notes on the new Higgs boson search by DZERO</title>
		<link>http://dorigo.wordpress.com/2009/03/02/notes-on-the-new-higgs-boson-search-by-dzero/</link>
		<comments>http://dorigo.wordpress.com/2009/03/02/notes-on-the-new-higgs-boson-search-by-dzero/#comments</comments>
		<pubDate>Mon, 02 Mar 2009 14:17:16 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[D0]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[neural networks]]></category>
		<category><![CDATA[standard model]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2100</guid>
		<description><![CDATA[Three weeks ago the DZERO collaboration published new results of their low-mass Higgs boson search. This is about the production of Higgs bosons in association with a W boson, with the subsequent decay of the Higgs particle to a pair of b-quark jets, and the decay of the W to an electron-electron neutrino or muon- [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2100&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Three weeks ago the DZERO collaboration <a href="http://www-d0.fnal.gov/Run2Physics/WWW/results/prelim/HIGGS/H65/">published</a> new results of their low-mass Higgs boson search. This is about the production of Higgs bosons in association with a W boson, with the subsequent decay of the Higgs particle to a pair of b-quark jets, and the decay of the W to an electron-electron neutrino or muon- muon neutrino pair: in symbols, what I mean is <img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+WH+%5Cto+e+%5Cnu_e+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to WH \to e \nu_e b \bar b' title='p \bar p \to WH \to e \nu_e b \bar b' class='latex' />, or <img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+WH+%5Cto+%5Cmu+%5Cnu_%7B%5Cmu%7D+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to WH \to \mu \nu_{\mu} b \bar b' title='p \bar p \to WH \to \mu \nu_{\mu} b \bar b' class='latex' />. I wish to describe this important new analysis today, but first let me make a point about the reaction above.</p>
<p>In order to make this blog more accessible than it would otherwise be, I frequently write things inaccurately: precision is usually pedantic and distracting. But here I beg you to please note a detail I will not gloss over for once: to be accurate, one should write <img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+WH+%2B+X&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to WH + X' title='p \bar p \to WH + X' class='latex' />&#8230;, because what we care for is <span style="color:#ff0000;"><em>inclusive production</em></span> of the boson pair. If we omit the X, strictly speaking we are implying that the two protons annihilated into the two bosons, with exactly nothing else coming out of the collision. While that reaction is possible, it is ridiculously rare -actually, the annihilation into ZH is possible, while the one into WH does not conserve electric charge and is strictly forbidden. Anyway, bringing along a symbol to remind ourselves of the fact that our projectiles are like garbage bags, which fill our detectors with debris when we throw them at one another, is cumbersome and annoying, while accurate. I hope, however, you realize that this is an important detail: Higgs bosons at a hadron collider are always accompanied by debris from the dissociating projectiles.</p>
<p><strong>Two words on associated WH production and its merits<br />
</strong><br />
The associated production of the Higgs together with a W boson is the <span style="color:#ff0000;">&#8220;golden&#8221; signature</span> for low-mass Higgs hunters at the Tevatron collider. While producing the Higgs together with another heavy object is not effortless (you are required to produce the collision with more energetic quarks in the two colliding protons, and this makes the production less frequent), the W boson pays back with extra dividends by producing a <span style="color:#0000ff;">very clean signature in its leptonic decay</span>, and by allowing the event to be spotted easily by the online triggering system, and collected with high efficiency by the data acquisition.</p>
<p>If you compare the collection of WH events to the collection of directly produced Higgs bosons (<img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+H+%2BX&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to H +X' title='p \bar p \to H +X' class='latex' />, where again I prefer accuracy by specifying the X), you immediately see the advantage of the former: while their production rate is four times smaller and the leptonic W decay only occurs 20% of the times, this 0.25 x 0.2=0.05=1/20 reduction factor is a<span style="color:#3366ff;"> <span style="color:#0000ff;">s</span></span><span style="color:#0000ff;">mall price to pay</span>, given the trouble one would have triggering on direct <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to b \bar b' title='H \to b \bar b' class='latex' /> events: the decay to a pair of b quarks is the dominant one for low Higgs boson masses, but the common nature of b-jets makes it unobservable.</p>
<p>Higgs decays to b-quark pairs produced alone simply cannot be triggered in hadronic collisions, because they are immersed in a background which is <span style="color:#ff0000;">six orders of magnitude higher</span> in rate, namely the production <img src='http://l.wordpress.com/latex.php?latex=p+%5Cbar+p+%5Cto+g+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='p \bar p \to g \to b \bar b' title='p \bar p \to g \to b \bar b' class='latex' /> of bottom-antibottom quark pairs by strong interactions. Even assuming that the online triggering system of DZERO were capable of spotting b-quark jet pairs with 100% purity (which is already a steep hypothesis), <span style="color:#0000ff;">the trigger would have to accept a million background events in order to collect just one fine signal event</span> !</p>
<p>Yes, life is tough for hadronic signatures at a hadron collider. Even finding the <img src='http://l.wordpress.com/latex.php?latex=Z+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Z \to b \bar b' title='Z \to b \bar b' class='latex' /> signal, which is a thousand times more frequent, is a tough business -it took CDF years to find a reasonable sample of those decays, while DZERO has not yet published anything on the matter. But the Tevatron experiments cannot ignore the fact that, if a low Higgs mass is hypothesized, the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to b \bar b' title='H \to b \bar b' class='latex' /> decay is the most frequent: the Higgs boson likes to decay into the heaviest pair of particles it can produce. If the total mass of a pair of W bosons or Z bosons is too heavy, the next-heaviest pair of decay products is b-quarks. This dictates the need to search for <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to b \bar b' title='H \to b \bar b' class='latex' />, and the trouble of triggering on such a process in turn makes the associated WH (or ZH) production the most viable signal.</p>
<p><strong>The DZERO analysis<br />
</strong><br />
The new analysis by DZERO studies a total integrated luminosity of 2<span style="color:#0000ff;">.7 inverse femtobarns</span>. This corresponds to <span style="color:#ff0000;">150 trillion proton-antiproton collisions</span>, but DZERO has netted almost twice as much data already by now, and it is only a matter of time before those too get included in this search: so one has to bear in mind that the statistical power of the data is soon going to increase by about 40%: the data increase corresponds to an increase in precision by the square root of two, or a factor of 1.41.</p>
<p>DZERO selects events which have an electron or a muon with high energy -the tag of a leptonic decay of the W boson-, missing transverse energy, and two or three hadronic jets. The presence of a energy imbalance in the plane transverse to the beam direction is a comparatively clean signature of the escape of the energetic neutrino produced together with the charged lepton by the W decay, and two jets are expected from the decay of the Higgs boson to a pair of b quarks. However, <span style="color:#ff0000;">you might well ask, <em>quid opus fuit tertium</em> ?</span></p>
<p>No, I bet you would not ask it that way -for some reason, a reminescence of Latin sprung up in my mind. <em>Quid opus fuit tertium</em> &#8211; What is the matter with the third one ? The third jet is not specifically a signature of any one of the decay products of the WH pair we are after. However, if you remember what I mentioned above, we are searching for <span style="color:#0000ff;">inclusive production</span> of a WH pair: that means we accept the fact that the two projectiles also produced an additional energetic stream of hadrons in the final state. That possibility is by no means rare, and in fact it amounts to about 20% of the Higgs production events. <span style="color:#0000ff;">By selecting events with two or three jets, DZERO increases its acceptance of signal events sizably.</span></p>
<p>A technique which has become commonplace in the hunt of elusive subnuclear particles is to slice and dice the data: <span style="color:#ff0000;">categorizing events in disjunct classes</span> is a powerful analysis strategy. By taking two-jet events on one side, and three-jet events on the other, DZERO can study them separately, and appreciate the different nuisances of each class. In fact, they further divide the data into subsets where one jet was tagged as a b-quark-originated one, or two of them were.</p>
<p>And they also keep separated the electron+jets and the muon+jets events: this also does make sense, since the experimental signatures of electrons and muons are slightly different, as are the resulting energy resolutions. <span style="color:#0000ff;">In total, one has eight disjunct classes</span>, depending on the number of jets, the number of b-tags, and the lepton species.</p>
<p>In order to decide whether there is a hint of Higgs bosons in any of the classes, backgrounds are studied using Monte Carlo simulations of all the Standard Model processes which could contribute to the eight selected signatures. These include the production of a W boson plus hadronic jets (&#8220;<span style="color:#0000ff;">W+jets</span>&#8220;) as well as the production of<span style="color:#0000ff;"> top quark pairs</span>: both these processes produce energetic leptons in the final state; but another background is due to events which do not actually contain a lepton, and where a hadronic jet was mistook for one. The latter is called &#8220;<span style="color:#0000ff;">QCD background</span>&#8221; highlighting its origin in strong interaction processes yielding just hadronic jets: despite the rarity of a jet faking a energetic lepton, the huge rate of QCD events makes this background sizable.</p>
<p>Among the characteristics that can separate the WH signal from the above backgrounds, the identity of the parton originating the hadronic jets is a powerful one: b-jets are more rare than light-quark ones, but there must be two of them in a <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to b \bar b' title='H \to b \bar b' class='latex' /> decay. DZERO uses a neural network which employs seven discriminating variables to select jets with a likely b-quark content.</p>
<p>The good thing with a neural-network b-tagger is that <span style="color:#0000ff;">the output of the network can be dialed to decide its purity</span>. And in fact, DZERO does exactly that. They start with a loose selection which has a rate of &#8220;false positives&#8221; of 1.5% (light-quark jets that are classified as b-tagged). If two jets have such a loose b-tag, the event is classified as a &#8220;double b-tag&#8221;; otherwise, the NN output requirement is made tighter, and &#8220;single-b-tag&#8221; events are collected by requiring that the b-tag has a better purity, with a &#8220;false positive&#8221; rate of 0.5%. These cuts have been optimized for their combined sensitivity to the Higgs signal.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/H65F07d.jpeg" alt="" width="460" /></p>
<p>Apart from b-tags, the signal displays a <span style="color:#ff0000;">different kinematics</span> than all backgrounds. Again, seven variables are used, which now describe the event kinematics: the transverse energy of the second-leading jet, the angle between jets, the dijet invariant mass, and a <span style="color:#0000ff;">matrix-element discriminant</span>, which is computed by comparing the probability density of the quadrimomenta of the objects produced in the decay in a WH event to that of backgrounds. In the figure above, the matrix element discriminant is shown for all the processes contributing to the class of W+2jet events with two b-tags. The output of the neural network shows that Higgs events fall in the right-side of the distribution, while backgrounds pile up mostly on the left, as can be seen in the figure below.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/H65F08d.jpeg" alt="" width="460" /></p>
<p><strong>Results of the search</strong></p>
<p>Since no signal is observed in the NN output distribution seen in the data, DZERO proceeds to set upper limits on the signal cross-section. For 2-jet events they use the NN output is used, while they use the dijet mass distribution for the 3-jet event classes. No justification is provided in their paper for this choice, which looks slightly odd to me, but I imagine they have done some optimization studies before taking this decision. However, I would imagine that the NN output is in principle always more discriminant than just one of the variables on which the network is constructed&#8230; Maybe somebody from DZERO could clarify this point in the comments thread, to the benefit of the other readers ?</p>
<p>At the end of the day, DZERO obtains limits on the cross section of the searched signal, which are still above the standard model predictions whatever the Higgs mass: therefore, they do not provide an exclusion of mass values, yet. These results, however, once combined with other results from CDF and DZERO, will one day directly imply that a SM Higgs cannot exist, if its mass is in a specified range. In the graph below you can see the limit set by this analysis on the WH production cross-section as a function of Higgs mass.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/H65F10b.jpeg" alt="" width="460" /></p>
<p>The black curve shows the 95% exclusion, while the hatched red curve shows the result that DZERO was expecting to find, based on pseudoexperiments. The comparison of the two curves is not terribly informative, but it does show that there were not surprises from the data.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/llr_d0wh27fb.jpg" alt="" width="461" height="293" /></p>
<p>The result can also be shown in the standard &#8220;LLR plot&#8221; above, which is showing, again as a function of the Higgs boson mass, the log-likelihood ratio of two hypotheses: the &#8220;<span style="color:#ff0000;">background only</span>&#8221; and the &#8220;<span style="color:#ff0000;">signal+background</span>&#8221; one. Let me explain what that is. For each mass value on the x-axis, imagine the Higgs is there. Then, <em>with large statistics, the data would show a propension for the &#8220;signal plus background&#8221; hypothesis, and the LLR would be large and negative</em>. If, instead, the Higgs did not exist at any mass value, the LLR would be large and positive. The two hypotheses can be run on pseudo-data of the same statistical power as the data really collected, thus producing the red and black hatched lines in the plot below. The two curves are different, but the red one does not manage to depart from the green band constructed around the black hatched one: that means that <em>the data size and the algorithms used in the analysis do not have enough power to discriminate the two hypotheses</em>, not even at 1-sigma level (which is the meaning of the width of the green band, while the yellow one shows two-sigma contours). The full black line shows the behavior of real data: they have a propension of confirming the background-only hypothesis at low mass, and a slight penchant for the signal+background one at about 130 GeV. But this is a really, really small fluctuation, well within the one-sigma band!</p>
<p>I think the LLR plot is a great way to describe the results of the search visually. It at once tells you the power of the analysis and the available data, and the outcome on the real events collected. Now, it takes twenty thick lines of text to explain it, but once you&#8217;ve grabbed its meaning&#8230;</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2100/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2100/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2100/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2100/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2100/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2100/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2100/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2100/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2100/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2100/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2100&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/03/02/notes-on-the-new-higgs-boson-search-by-dzero/feed/</wfw:commentRss>
		<slash:comments>6</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/H65F07d.jpeg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/H65F08d.jpeg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/H65F10b.jpeg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/llr_d0wh27fb.jpg" medium="image" />
	</item>
		<item>
		<title>Anybody with an AAAS subscription willing to do me a favor ?</title>
		<link>http://dorigo.wordpress.com/2009/02/20/anybody-with-an-aaas-subscription-willing-to-do-me-a-favor/</link>
		<comments>http://dorigo.wordpress.com/2009/02/20/anybody-with-an-aaas-subscription-willing-to-do-me-a-favor/#comments</comments>
		<pubDate>Fri, 20 Feb 2009 17:04:09 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[personal]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[journalism]]></category>
		<category><![CDATA[LHC]]></category>
		<category><![CDATA[science outreach]]></category>
		<category><![CDATA[science reporting]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2075</guid>
		<description><![CDATA[Here I am, once again improperly and shamelessly using this public arena for my personal gain. This time, I need help from one of you who has a subscription to the American Association for the Advancement of Science.
It so happens that a couple of weeks ago I gave a phone interview to Adrian Cho about [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2075&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Here I am, once again improperly and shamelessly using this public arena for my personal gain. This time, I need help from one of you who has a subscription to the <a href="http://www.aaas.org/aboutaaas/">American Association for the Advancement of Science</a>.</p>
<p>It so happens that a couple of weeks ago I gave a phone interview to Adrian Cho about the LHC, the Tevatron, and the hunt for the Higgs boson. We discussed various scenarios, the hunt going on at the Tevatron, and other stuff. I am curious to know what Adrian made of our half-hour chat. Today, I realized that <a href="http://www.sciencemag.org/cgi/content/short/323/5917/993"> the article has been published</a>, but I have no access to the it, since it is available at the Science Magazine site only for AAAS members.</p>
<p>I have to say, Adrian should have been kind enough to forward me a copy of the piece that benefitted from the interiew. I am sure he forgot to do it and once he reads this he will regret it, or maybe he thinks I am a member of the AAAS already&#8230; Adrian, you are excused. But this leaves me without the article for a while, and I am a curious person&#8230; So if you have an AAAS account and you are willing to break copyright rules, I beg you to send me a file with the article! My email is dorigo (at) pd (dot) infn (dot) it. Thank you!</p>
<p>And, to show you just how serious I am when I say I am shameless, here&#8217;s more embarassment:<em> if you  are a big shot of the AAAS, do you by any chance give free membership to people who do science outreach to the sole benefit of the advancement of Science  ? </em></p>
<p><strong>UPDATE:</strong> I am always amazed by the power of internet and blogging. These days you just have to ask and you will be given! So, thanks to Peter and Senth, I got to read the article by Adrian Cho.</p>
<p>I must admit I am underwhelmed. Not by the article, which is incisive and to the point. Only, I should know that science journalists quote you for 1% of what you tell them, and use the rest to get informed and write a better piece. In fact, the piece starts by quoting me:</p>
<blockquote><p>“Three years ago, nobody would have bet a lot that the Tevatron<br />
would be competitive [with the LHC] in the Higgs search. Now I think the tables are almost turned,” says Tommaso Dorigo, a physicist from the University of Padua in Italy who works with the CDF particle detector fed by the Tevatron and the CMS particle detector fed by the LHC.</p></blockquote>
<p>&#8230; but that is the only quote. I can console myself by noting I am in quite good company: experiment spokespersons, Fermilab director Pier Oddone, CERN spokesperson James Gillies&#8230;</p>
<p><em><br />
</em></p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2075/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2075/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2075/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2075/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2075/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2075/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2075/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2075/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2075/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2075/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2075&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/02/20/anybody-with-an-aaas-subscription-willing-to-do-me-a-favor/feed/</wfw:commentRss>
		<slash:comments>3</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>The 1999/2003 Higgs predictions compared with CDF 2009 results</title>
		<link>http://dorigo.wordpress.com/2009/02/13/the-19992003-higgs-predictions-compared-with-cdf-2009-results/</link>
		<comments>http://dorigo.wordpress.com/2009/02/13/the-19992003-higgs-predictions-compared-with-cdf-2009-results/#comments</comments>
		<pubDate>Fri, 13 Feb 2009 14:02:18 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[personal]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[D0]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2062</guid>
		<description><![CDATA[Two years ago I used the combined Higgs search limits produced by the D0 experiment to evaluate how well the Tevatron was doing if compared with the predictions that had been put together by the 1999 SUSY-HIGGS working group, and later by the 2003 Higgs Sensitivity Working Group (HSWG), two endeavours to which I had [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2062&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><a href="http://dorigo.wordpress.com/2007/05/03/the-2003-higgs-discovery-predictions-tested-with-hard-data/">Two years ago</a> I used the combined Higgs search limits produced by the D0 experiment to evaluate how well the Tevatron was doing if compared with the predictions that had been put together by the <a href="http://arxiv.org/PS_cache/hep-ph/pdf/0010/0010338.pdf">1999 SUSY-HIGGS working group</a>, and later by the <a href="http://www-d0.fnal.gov/Run2Physics/higgs_sensitivity_study.html">2003 Higgs Sensitivity Working Group</a> (HSWG), two endeavours to which I had participated with enthusiasm. The picture that emerged was that, although results were falling short of justifying fully the early predictions, there was still hope that those would one day be vindicated.</p>
<p>Indeed, I remember that when in 2003 the HSWG produced its <a href="http://www-d0.fnal.gov/Run2Physics/public/higgs/HSS_D0_CDF.pdf">report</a>, we felt our results were greeted with a dose of scepticism. And we ourselves were a bit embarassed, because we knew we had been a bit optimistic in our predictions: however, that was the name of the game &#8211; looking at things on their bright side, for the sake of convincing funding agents that the Tevatron had a reason to run for a long time. I felt a strong justification for being optimistic in the incredible results on the top quark mass that the Tevatron had already started achieving: early prospects of measuring the top mass to a 1% uncertainty have in fact been surpassed by the combination of dedication of the scientists doing the analyses, and their imagination in inventing new precise methods.</p>
<p>We now have a chance to look back at the 1999/2003 predictions for the Higgs reach of the Tevatron with a rather solid set of hard data: the CDF combination, which I <a href="http://dorigo.wordpress.com/2009/02/11/new-cdf-combination-of-higgs-limits/">briefly discussed two days ago</a>, is based on analyzed sets of data ranging from <span style="color:#ff0000;">2 to 3 inverse femtobarns</span>, and the comparisons do not require a lot of extrapolations to be carried out.</p>
<p><img style="width:450px;height:300px;" src="http://www.pd.infn.it/~dorigo/hswgpred.jpg" alt="" width="450" height="300" align="absbottom" /></p>
<p>If we look at the 1999/2003 predictions shown above (two basically coincident results, if one considers that the 2003 results were not accounting for systematic effects, which would worsen a bit the curves of sensitivity and bring them to match the older ones), we can <span style="color:#ff0000;">read off the integrated luminosity that the Tevatron experiments needed to analyze in order to exclude, by combining their results, SM Higgs production at 95% confidence level</span>. These numbers are as follows: for a Higgs mass of 100 GeV, <strong>1/fb</strong> was considered sufficient; for a Higgs mass of 120 GeV, <strong>2/fb</strong> were needed; <strong>10/fb</strong> at 140 GeV; <strong>4.5/fb</strong> at 160 GeV; <strong>8/fb</strong> at 180 GeV; and <strong>80/fb</strong> at 200 GeV. You can check them on the purple band in the graph above.</p>
<p>Now, let us take the actual expected limits by CDF with the analyses and the data they have based their new result upon (using expected limits rather than observed ones is correct, since the former are unaffected by statistical fluctuations). At 100 GeV, CDF has a reach in the 95%CL limit at 2.63xSM; at 120 GeV, the reach is 3.72xSM; at 140 GeV, 3.61xSM; at 160 GeV it is 1.75xSM; at 180 GeV 3.02xSM; and at 200 GeV, the reach is at 6.33xSM.</p>
<p>(<em>Below, the 2009 combined CDF limits are shown by the thick red curve; the data I list above is based on the hatched curve instead, which shows the expected limit.</em>)</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/collectedlimits16jan09.gif" alt="" width="460" /></p>
<p><strong>How do we now compare these sets of numbers ?</strong></p>
<p>Easy. As easy as 1.2.3.4 (well, not too easy, but that&#8217;s how it goes).</p>
<ol>
<li>We first <span style="color:#ff0000;">scale up by a factor of two</span> the 1999/2003 luminosity numbers needed for a 95% CL exclusion, which we listed above. We thus get, for Higgs masses ranging from 100 to 200 GeV in 20-GeV steps, needed integrated luminosities of <strong>2,4,20,9,16,160/fb</strong>.</li>
<li>Then, <span style="color:#ff0000;">we take the actual luminosity used by CDF</span> for the analyses that have been combined to yield the expected limits listed above. This is slightly tricky, since the combination includes analyses which have used 2.0/fb of data (the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+%5Ctau+%5Ctau&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to \tau \tau' title='H \to \tau \tau' class='latex' /> search), 2.1/fb (the <img src='http://l.wordpress.com/latex.php?latex=VH+%5Cto+ME_T+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='VH \to ME_T b \bar b' title='VH \to ME_T b \bar b' class='latex' /> search), 2.7/fb (the <img src='http://l.wordpress.com/latex.php?latex=WH+%5Cto+l+%5Cnu+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='WH \to l \nu b \bar b' title='WH \to l \nu b \bar b' class='latex' />, the <img src='http://l.wordpress.com/latex.php?latex=ZH+%5Cto+ll+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='ZH \to ll b \bar b' title='ZH \to ll b \bar b' class='latex' />, and the <img src='http://l.wordpress.com/latex.php?latex=WH+%5Cto+WWW&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='WH \to WWW' title='WH \to WWW' class='latex' /> searches), and 3.0/fb (the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+WW&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to WW' title='H \to WW' class='latex' /> search). In principle, we should weight those numbers with the relative sensitivity of the various analyses, but <span style="color:#ff0000;">we can approximate it by taking an &#8220;average effective luminosity</span>&#8221; of <strong>2.4/fb</strong> for the 100 GeV Higgs search, <strong>2.7/fb</strong> for the 120 and 140 GeV points, and <strong>3.0/fb</strong> for the high-mass searches. This is appropriate, since the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+WW&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to WW' title='H \to WW' class='latex' /> search starts kicking in above 140 GeV.</li>
<li>We now have all the numbers we need: <span style="color:#0000ff;">we divide the expected luminosity needed for one experiment by the 1999/2003 study, found at point 1 above, by the effective luminosities found at point 2, and take the square root of that number</span>: this means <span style="color:#ff0000;">finding the &#8220;reduction factor&#8221; in the sensitivity that the actual CDF data suffers with respect to the data needed to exclude the Higgs boson</span>. We find a reduction factor of <strong>0.91, 1.22, 2.72, 1.73, 2.31, and 7.30</strong> for Higgs masses of 100,120,140,160,180, and 200 GeV respectively.</li>
<li>Now we are done. We can compare the &#8220;times the SM&#8221; limits of CDF with the numbers found at point 3 above. The ratio of the two says how much worse is CDF doing with respect to predictions, for each mass point. <span style="color:#ff0000;">We find that CDF is doing <strong>2.88</strong> times worse than predictions at 100 GeV; <strong>3.06</strong> times worse than predictions at 120 GeV; <strong>1.33</strong> times worse at 140 GeV; <strong>1.01</strong> times worse at 160 GeV; <strong>1.31</strong> times worse at 180 GeV; and <strong>0.87</strong> times worse (i.e., 1.15 times better!) at 200 GeV.</span></li>
</ol>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/cdf_higgs_reach_09.jpg" alt="" width="460" /></p>
<p>The results of point 4 are plotted on the graph shown above, where the x-axis shows the Higgs mass, and the y axis this &#8220;shame factor&#8221;. I have given a 20% uncertainty to the figures I computed, because of the rather rough way I extracted the numbers from the 1999/2003 prediction graph. If you look at the graph, you notice that the CDF experiment has kept its (our!) promise (points bouncing around a ratio of 1.0) with its high-mass searches, while low-mass searches still are a bit below expectations in terms of reach (3x worse reach than expected). It is not a surprise: at low Higgs mass, the searches have to rely on the <img src='http://l.wordpress.com/latex.php?latex=H+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='H \to b \bar b' title='H \to b \bar b' class='latex' /> final state, which is very difficult to optimize (vertex b-tagging, dijet mass resolution, lepton acceptance are the three things on which CDF has been spending hundreds of man-years in the last decade). Give CDF (and DZERO) enough time, and those points will get down to 1.0 too!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2062/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2062/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2062/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2062/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2062/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2062/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2062/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2062/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2062/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2062/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2062&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/02/13/the-19992003-higgs-predictions-compared-with-cdf-2009-results/feed/</wfw:commentRss>
		<slash:comments>21</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/hswgpred.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/collectedlimits16jan09.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/cdf_higgs_reach_09.jpg" medium="image" />
	</item>
		<item>
		<title>New CDF Combination of Higgs limits!</title>
		<link>http://dorigo.wordpress.com/2009/02/11/new-cdf-combination-of-higgs-limits/</link>
		<comments>http://dorigo.wordpress.com/2009/02/11/new-cdf-combination-of-higgs-limits/#comments</comments>
		<pubDate>Wed, 11 Feb 2009 17:46:05 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LHC]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=2055</guid>
		<description><![CDATA[A brand-new combination of Higgs boson cross-section limits has been recently produced by the CDF experiment for the 2009 winter conferences. The results are almost one month old, but I decided to wait a bit before posting them here, in order to avoid arising bad feelings in a few of my CDF colleagues, those who [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2055&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>A brand-new combination of Higgs boson cross-section limits has been recently produced by the CDF experiment for the 2009 winter conferences. The results are almost one month old, but I decided to wait a bit before posting them here, in order to avoid arising bad feelings in a few of my CDF colleagues, those who believe I have no right to post here published results in too timely a fashion, because they feel those results should first be presented at conferences by the real authors of the analyses.</p>
<p>Now I think it is due time to have the most relevant plots here, since they are all available from a <a href="http://www-cdf.fnal.gov/physics/new/hdg/results/combcdf_090116/">public web page</a> of CDF anyway; so here we go, with the most updated information. Mind you, these are CDF-only results: a sizable improvement in the limits will come when they get combined with the findings of DZERO. I seem to understand that the Tevatron combination group folks are dragging their feet this year, so we have better to just as well take the CDF results and comment them alone.</p>
<p>The first graph is the most important one of all: it describes the combination of CDF results, in the usual &#8220;95% CL limit on <em>times the SM cross section</em>&#8220;. It is shown below.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/collectedlimits16jan09.gif" alt="" width="460" /></p>
<p>On the x axis is the Higgs boson mass, and on the y axis the cross-section limit. Different colors of the curves refer to different analyses, which target the various decay channels of the sought particle; hatched lines show expected limits, and full ones show instead the limits actually obtained by the analysis.</p>
<p>As you can see by examining the thick red curve at the bottom, CDF by itself cannot rule out the 170-GeV point, which last summer was excluded by the CDF+D0 combination. However, <span style="color:#ff0000;">a sizable improvement can be observed across the board in the results</span>. The red curve, for one thing, is considerably flatter than it used to be, a sign that the low-mass searches have started to pitch in with momentum. Another thing to note is that these results correspond to 3.0/fb of analyzed luminosity or less (2.4/fb at low mass): there is already at least twice as much data waiting to be analyzed, and results are thus expected to sizably improve their sensitivity.</p>
<p>The above summary brings me to mention another important point. By looking at the graph, you might run the risk of failing to appreciate the <span style="color:#ff0000;">enormous effort </span>which CDF is putting into these searches. In truth, the name of the game is not &#8220;wait more data and turn the crank&#8221;. Quite the opposite! The most important improvements in the discovery reach have been achieved in the course of the last five years by <span style="color:#ff0000;">continuously improving the algorithms</span>, the search methods, by refining tools, by finding new avenues of investigation, and new search channels neglected before. This is summarized masterfully in the two graphs shown below.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/cdf115jan09log.gif" alt="" width="460" /></p>
<p>Above, you can see that for a Higgs mass of 115 GeV, the limit that CDF was able to set on its existence, in terms of cross section (well, &#8220;times the SM cross section&#8221; units to be precise: the ones shown on the y axis) has <strong>improved much more</strong> than what one would have expected by scaling down the limit with a simple square root law -the one that Poisson Statistics would dictate, for statistically-limited measurements. Quite the opposite: as time went by, the actual limits (colored points) have moved down almost vertically, a sign that the data has been used better and better! Above, if you took the extrapolation expected after the first limit was published (the one in green), you would expect that the limit today, with 2.4/fb analyzed, was at 7xSM, while it in fact is at 3xSM: this corresponds to a 2.3x improvement in the limit, which would have been granted by a 5.2 times larger analyzed dataset!!</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/cdf160jan09log.gif" alt="" width="460" /></p>
<p>Above, the same information is shown for the <img src='http://l.wordpress.com/latex.php?latex=M_H+%3D+160+GeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_H = 160 GeV' title='M_H = 160 GeV' class='latex' /> value. In this case, CDF is now expected to be able to set an exclusion alone with 9/fb of data, but we still expect to see some improvements in the data analyses, which should move the points well into the brown band. In this case, 7/fb of data might be enough.</p>
<p>The last two plots I wish to discuss are shown below. <strong>BEWARE:</strong> This is information that LHC scientists would really, really not like to see &#8211; so, if your life depends on the success of ATLAS or CMS, please stop reading now, take my advice.</p>
<p>OK. The plot below shows the probability that the Tevatron experiments, by combining their datasets and results, may observe a 2-sigma evidence for SM Higgs production, with 5/fb and 10/fb of data collected by each. If the analyses will not perform better than what they have so far, you get the full lines -red for 5/fb, blue for 10/fb. If they improve as much as it is reasonable to predict, you get the hatched lines.</p>
<p>What to gather from the plot ? Well: it seems that, regardless of the Higgs boson mass, the Tevatron has a sizable chance to be able to say something good, by the time CDF and D0 will have analyzed the datasets they already possess (which are in excess of 5/fb each: the delivered luminosity of the Tevatron is passing the 6/fb mark as we speak, and the typical live time of the experiments is above 80%).</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/twosig2xcdf_ykk_impnoimp_510fb.gif" alt="" width="460" /></p>
<p>Below, we see what is the chance of a 3-sigma evidence. Again, there is a sizable chance of that happening, although if no additional improvements occur in the analyses, it seems that the Tevatron will need to get lucky!</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/threesig2xcdf_ykk_impnoimp_510fb.gif" alt="" width="460" /></p>
<p>I remember that in 2005 I gave a talk in Corfù (Greece) where I ventured to speculate on the possible scenarios for Higgs searches at the Tevatron and the LHC. One of the scenarios saw the two experiments competing to find the particle with roughly equal reach, and eventually producing a combined observation. That possibility  does not seem too far-fetched any longer!</p>
<p>In the next few days I plan to discuss in some detail the most important analyses which contribute to the combination discussed above. Stay tuned&#8230;</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/2055/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/2055/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/2055/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/2055/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/2055/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/2055/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/2055/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/2055/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/2055/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/2055/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=2055&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/02/11/new-cdf-combination-of-higgs-limits/feed/</wfw:commentRss>
		<slash:comments>22</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/collectedlimits16jan09.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/cdf115jan09log.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/cdf160jan09log.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/twosig2xcdf_ykk_impnoimp_510fb.gif" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/threesig2xcdf_ykk_impnoimp_510fb.gif" medium="image" />
	</item>
		<item>
		<title>Single top seen with no leptons!</title>
		<link>http://dorigo.wordpress.com/2009/01/14/single-top-seen-with-no-leptons/</link>
		<comments>http://dorigo.wordpress.com/2009/01/14/single-top-seen-with-no-leptons/#comments</comments>
		<pubDate>Wed, 14 Jan 2009 15:42:41 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[personal]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[missing energy]]></category>
		<category><![CDATA[Purdue]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top mass]]></category>
		<category><![CDATA[top quark]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1948</guid>
		<description><![CDATA[This post has a rather long introduction which does not discuss single top production, but rather explains how the techniques for detecting top quark pairs at the Tevatron have evolved since the first searches. Informed readers who are interested mainly in the new CDF result for the single top cross section may skip the first [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1948&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>This post has a rather long introduction which does not discuss single top production, but rather explains how the techniques for detecting top quark pairs at the Tevatron have evolved since the first searches. Informed readers who are interested mainly in the new CDF result for the single top cross section may skip the first two sections below&#8230;</p>
<p><strong>Introduction: missing energy as the main tag top quarks </strong></p>
<p><img src="http://www.pd.infn.it/~dorigo/stmetjj_dil.jpg" border="0" alt="" align="none" /></p>
<p>In the years before the top quark discovery, and for a few years thereafter, top quark pairs produced by the Tevatron proton-antiproton collider were searched by the CDF and D0 experiments with a quite clear, if a bit unimaginative, three-pronged strategy.</p>
<p><img src="http://www.pd.infn.it/~dorigo/stmetjj_std.jpg" border="0" alt="" align="right" /> A top quark pair candidate event could be extracted from backgrounds if it contained two charged leptons -basically electrons or muons-, missing transverse energy, and two hadronic jets (the <span style="color:#ff0000;">dilepton signature</span>, pictured above); or if there were one charged lepton, missing transverse energy, and three or four hadronic jets (the<span style="color:#ff0000;"> single-lepton signature</span>, shown on the right); or finally, if it just showed six hadronic jets (the <span style="color:#ff0000;">all-hadronic signature</span>).</p>
<p>(<em>A note to avoid letting down from square one those of you who feel inadequate for not knowing what a jet, or missing energy, are: Jets are the result of the materialization of high-energy quarks, which are kicked out of the colliding protons or materialized by the released energy, into streams of hadronic particles; they appear in collider detectors as localized deposits of energy. Missing energy results from the escape of undetected particles, typically neutrinos. More on this below&#8230;</em>)</p>
<p>The three final states mentioned above were the result of the <span style="color:#ff0000;">different decay modes of the two W bosons</span> always present in a top pair decay: if both W bosons decayed to lepton-neutrino pairs one would get a dilepton event; if one decayed to a lepton-neutrino and the other to a pair of hadronic jets the single-lepton final state would arise; and if both decayed to jets one would get the six-jet topology. Life in the top physics group was just that easy.</p>
<p>The dilepton final state is the cleanest of the three channels, and the all-hadronic final state the dirtiest: in proton-antiproton collisions a simple rule of thumb states that <span style="color:#0000ff;">the more leptons you are after, the cleaner your signal is</span>, and conversely the more jets you look for, the deeper you have to dig in the mud of strong interactions. That is because strong interactions (or QCD, for Quantum ChromoDynamics) produce lots and lots of jets, and very rarely do they yield leptons; and QCD is the name of the game in proton-antiproton collisions.</p>
<p>It took quite a while to realize that one could imagine other successful ways to extract top-quark pairs from Tevatron data. A sizable step forward on this issue was made by yours truly with the help of a graduate student, I am proud to note. Let me explain this in a few lines.</p>
<p>While the search for leptons (electrons, muons, tauons) is a way to clean the dataset from QCD backgrounds, the explicit identification of these particles results by force in a <span style="color:#ff0000;">reduction of the available top signal</span>. The CDF and D0 experiments are well-suited to detect electrons and muons, but only when these particles are produced at a large angle from the proton beam axis -i.e., &#8220;centrally&#8221;; moreover, the lepton identification efficiency is never 100% even in those cases. As for tauons, they are much harder to detect, because the tauon is a heavy particle, so that despite being a lepton it has the chance to decay into light hadrons, mimicking a hadronic jet.</p>
<p>All in all, if one considers the single-lepton final state of the process <img src='http://l.wordpress.com/latex.php?latex=t+%5Cbar+t+%5Cto+W%5E%2B+b+W%5E-+%5Cbar+b+%5Cto+l+%5Cnu+b+q+%5Cbar+q%27+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='t \bar t \to W^+ b W^- \bar b \to l \nu b q \bar q&#039; \bar b' title='t \bar t \to W^+ b W^- \bar b \to l \nu b q \bar q&#039; \bar b' class='latex' />, which arises in a total of 44% of the cases, the typical fraction of top pair decays one may hope to collect in a clean dataset is <strong>not larger than 10%</strong>. The rest is lost when one explicitly requires to have reconstructed a central, clean lepton signal.</p>
<p>Put this way, it does beg the question. What are we going to do with the large fraction of lost top pair decays ? The answer, for eight years after the top discovery, was simple: nothing. There had been, in truth, attempts at loosening the identification requirements on leptons; but the fact that leptons are the means by which those events are collected -they are requested by the online triggering system- called for a more radical solution. So Giorgio Cortiana and I, while looking for a suitable thesis topic for him, decided to <span style="color:#ff0000;">drop the lepton request altogether</span>, and to simply look for top pairs in data just containing missing transverse energy and jets.</p>
<p><span style="color:#0000ff;">Missing transverse energy</span> is a powerful signature at hadron colliders by itself, because it may signal the presence of an energetic neutrino escaping the detector. The signature arises from a simple calculation of the energy flowing out of the interaction point in the plane transverse to the beam direction: in that plane, momentum conservation implies that the vector sum of all particles is zero, compatibly with measurement uncertainties: if it very different from zero, either one or more particles have escaped unnoticed, or some of them have been measured imprecisely.</p>
<p>If a significant amount of missing transverse energy effectively tags an energetic neutrino, <span style="color:#0000ff;">there is no need to search for an additional charged lepton to confirm that a leptonic <img src='http://l.wordpress.com/latex.php?latex=W+%5Cto+l+%5Cnu&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='W \to l \nu' title='W \to l \nu' class='latex' /> decay has taken place</span>! Energetic neutrinos are either due to a leptonic W decay or a Z boson decay to a pair of neutrinos, <img src='http://l.wordpress.com/latex.php?latex=Z+%5Cto+%5Cnu+%5Cnu&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Z \to \nu \nu' title='Z \to \nu \nu' class='latex' />. Now, Z bosons are even more rare than W bosons, so they do not constitute a too worrisome background. <em>By ignoring the charged lepton that might accompany the missing transverse energy, one gains access to all the bounty of single lepton decays of top quark pairs which the tight search discards</em> -because the charged lepton went unseen in a hole of the detector, or failed the identification criteria.</p>
<p>Giorgio and I published <strong>two papers</strong> using the missing-energy-plus-jets signature: a <a href="http://qd.typepad.com/6/2005/07/ok_so_i_promise.html">cross-section measurement for top-pair production</a> (<a href="http://www-cdf.fnal.gov/physics/preprints/cdf7963_metjets_ttbar_xsec_3.ps">paper here</a>) which, at the time of publication, was the third-best result on that quantity, and <a href="http://dorigo.wordpress.com/2007/05/08/new-paper-approved/">a top quark mass measurement</a> (<a href="http://www-cdf.fnal.gov/physics/preprints/cdf8684_metjets_mt_prdrc.ps">paper here</a>) which, despite carrying a large uncertainty, showed that the sample could be a promising ground for top physics measurements despite the lack of kinematic closure (the fact that one lepton is present but is unidentified means that one cannot completely define the decay kinematics: one then speaks of unconstrained kinematics). Now, I am glad to see that the same signature we used for top quark pairs is being exploited in CDF for a single top quark search.</p>
<p><strong>A few words on single top production<br />
</strong><br />
Single tops are produced in proton-antiproton collisions by <span style="color:#ff0000;">weak interaction processes</span>, but they are not much less frequent than strongly-produced top pairs,<br />
because a pair of top quarks weighs twice as much as a single top quark does, and this has a huge impact in the cross section. Usually, the single-top production signature amounts to the leptonic top decay products -a charged lepton, missing energy, and a jet- accompanied by another jet or two, produced by the quark(s) originally recoiling against the top quark. If one considers the simplest diagrams giving rise to a single top quark, there are two very different processes:<span style="color:#ff0000;"> s-channel<br />
W* decay</span> and <span style="color:#ff0000;">t-channle W-gluon fusion</span>. Let me explain what these are.</p>
<p>A regular, &#8220;on-shell&#8221; W boson -one which has a mass very close to the peak of the W<br />
resonance, <img src='http://l.wordpress.com/latex.php?latex=M_W%3D80.4+GeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_W=80.4 GeV' title='M_W=80.4 GeV' class='latex' />- does not decay into a top and a bottom quark: that is because the W is lighter than the required final state particles! But a W boson produced &#8220;off-mass-shell&#8221;, i.e. with a mass much larger than its normal value, can indeed decay that way. One just has to remember that W bosons may have any mass from 0 to whatever value, but the probability that the mass is far from <img src='http://l.wordpress.com/latex.php?latex=M_W&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='M_W' title='M_W' class='latex' /> quickly becomes small, following a curve called a Breit-Wigner; one I have <a href="http://dorigo.wordpress.com/2008/12/19/more-on-the-z-lineshape-at-lhc/">recently posted</a> in a discussion about Z bosons, incidentally. You can check the shape there, bearing in mind that the peak for W bosons is 10 GeV smaller, and the width about 20% smaller. Anyway, when a off-mass-shell W boson decays as <img src='http://l.wordpress.com/latex.php?latex=W+%5Cto+t+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='W \to t \bar b' title='W \to t \bar b' class='latex' />, as shown in the diagram on the right in the figure below, <span style="color:#0000ff;">the final state ends up containing two b-quarks, plus the decay products of the second W boson appearing in the process</span> -the one emitted by the top decay. So one has a lepton, missing transverse energy, and two b-jets.</p>
<p><img src="http://www.pd.infn.it/~dorigo/singletop.jpg" border="0" alt="" width="450" height="267" align="absbottom" /></p>
<p>The second way by means of which a single top quark may be produced in proton-antiproton collisions is shown on the left above, and it occurs via the <span style="color:#ff0000;">splitting of a gluon from the proton into a bottom-antibottom quark pair</span>: while one of them does not concern us, the other interacts with a W boson emitted from the other projectile, and a top quark is the result. One thus obtains the signature of <strong>three jets plus lepton plus missing transverse energy</strong>, and two of the jets still have b-quarks in them.</p>
<p><strong>The new CDF result</strong></p>
<p>Single top production has been sought at the Tevatron with enthusiasm in Run II, and CDF and D0 have already shown sizable signals of that process in datasets containing leptons, missing energy, and jets. But finally, a new analysis by the <span style="color:#ff0000;">Purdue University</span> group in CDF (Artur Apresyan, Fabrizio Margaroli, and Karolos Potamianos, led by Daniela Bortoletto) is now finding a signal without the help of the charged lepton. I of course cannot but be happy about it, since it is just another demonstration of the potentiality of the &#8220;lepton-ignoring&#8221; technique!</p>
<p>The new analysis selects events with a significant amount of missing transverse energy (<img src='http://l.wordpress.com/latex.php?latex=ME_T%3E50+GeV&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='ME_T&gt;50 GeV' title='ME_T&gt;50 GeV' class='latex' />) accompanied by two or three hadronic jets. Events are not collected as signal candidates if the missing Et has a small azimuthal angle with a jet, because that is a hint that the former may be due to a fluctuation of the energy measurement of the latter. After that selection, a combination of b-quark tagging algorithms is used to select a sample rich with two b-quark jets -the other important background-reducing characteristic of top decays.</p>
<p><span style="color:#0000ff;">Three different classes of b-enriched events are selected.</span> Two classes depend solely on the presence in the jets of one or two &#8220;<strong>Secvtx</strong>&#8221; b-tags: these are explicitly reconstructed secondary vertices, signalling the decay in flight of a B-hadron. A third class collects events with one Secvtx b-tag plus a jet tagged by a different algorithm, &#8220;<strong>JetProb</strong>&#8220;. JetProb computes the probability that charged tracks contained in a jet originate from the primary vertex, and tags jets which are likely to contain a long-lived particle.</p>
<p>The three classes have a different signal purity, and their separate analysis allows to extract more information from the data sample than a combination of all b-tagged events.</p>
<p>A neural-network classifier is used to discriminate single-top events from the surviving backgrounds, which are predominantly due to a combination of three processes: &#8220;<span style="color:#ff0000;">W+jets&#8221; production</span>, which arises when a W boson is created along with QCD radiation; <span style="color:#ff0000;">top pair production</span>, which does produce missing energy and b-tagged jets, but has typically a larger number of jets; and the more generic <span style="color:#ff0000;">QCD-multijet background</span>, which may contaminate the sample when missing transverse energy is faked by a weird fluctuation in the energy measurement of one of the hadronic jets, not removed by the azimuthal angle cuts mentioned above. Since the latter is the largest offender, this neural network -through the choice of kinematical variables- is aimed in particular at downsizing QCD events.</p>
<p><img src="http://www.pd.infn.it/~dorigo/stmetjj_nn1.jpg" border="0" alt="" align="absbottom" /></p>
<p>Above you can see the NN output for the class of events containing two Secvtx b-tags; points with error bars are the data, and the expected backgrounds are shown by color-coded histograms. The QCD background (in green) populates the negative region, as expected.</p>
<p>After the selection of high-NN-output events  (<img src='http://l.wordpress.com/latex.php?latex=NN%3E-0.1&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='NN&gt;-0.1' title='NN&gt;-0.1' class='latex' />), about a thousand events survive in the &#8220;one Secvtx&#8221; class, and about a hundred in the &#8220;two Secvtx&#8221; and &#8220;one Secvtx-one JetProb&#8221; class. The first class is dominated by QCD backgrounds, while the second and the third have top pairs as the main contribution. These backgrounds are precisely estimated using a <span style="color:#0000ff;">tagging-matrix approach</span>: a parametrization of the probability of finding b-tags in jets as a function of the jet characteristics. Control samples of data are used to verify that the background expectations are accurate.</p>
<p>The analysis does not end there, though: the single top signal is small, and the samples have to be purified further. The authors use <span style="color:#ff0000;">another neural network</span>, trained with variables sensitive to the signal kinematics, and extract the signal size from the NN output distributions in the three different classes.</p>
<p>Below you can see the second-NN output for the first class of events. As you can see, the s-channel and t-channel single-top production processes are small, but the fit prefers to include them in the mixture.</p>
<p><img src="http://www.pd.infn.it/~dorigo/stmetjj_nn2.jpg" border="0" alt="" align="none" /></p>
<p>The graph below displays the results class by class, and the combination.</p>
<p><img src="http://www.pd.infn.it/~dorigo/stmetjj_res.jpg" border="0" alt="" align="none" /></p>
<p>The analysis finds a very nice result: <span style="color:#0000ff;">the single top cross section is measured at <img src='http://l.wordpress.com/latex.php?latex=%5Csigma_t+%3D+4.9%5E%7B%2B2.5+%7D_%7B-2.2%7D+pb&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\sigma_t = 4.9^{+2.5 }_{-2.2} pb' title='\sigma_t = 4.9^{+2.5 }_{-2.2} pb' class='latex' /></span>, in good agreement with standard model expectations. The measured significance of the signal is quoted at <img src='http://l.wordpress.com/latex.php?latex=2.1-%5Csigma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='2.1-\sigma' title='2.1-\sigma' class='latex' />, while the expected sensitivity of the search is given by the paper at <img src='http://l.wordpress.com/latex.php?latex=1.4-%5Csigma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='1.4-\sigma' title='1.4-\sigma' class='latex' />: this is a very important number to quote, as it allows one to size up with precision the relative importance of this determination, decoupling from statistical fluctuation effects that may influence the particular value found by the analysis.</p>
<p>Given the fact that it is based on a data sample orthogonal to others, once combined with the other determinations the new measurement described above will give a <span style="color:#ff0000;">sizable contribution to the significance of the CDF signals</span> of single top production: the authors must be heartily congratulated for their  result!</p>
<p>And the goodies are not over: the measurement of the cross section for single top production can be directly translated in a determination of the <span style="color:#0000ff;">$V_{tb}$ matrix element of the Cabibbo-Kobayashi-Maskawa matrix</span>. The plot below shows the result obtained by this search. Of course we are still far from a meaningful determination, and this also reflects in the unphysical value obtained, which is however in good agreement with the expectation, close to 1.0 in the standard model.<br />
<img src="http://www.pd.infn.it/~dorigo/stmetjj_vtb.jpg" border="0" alt="" align="absbottom" /></p>
<p>I have not seen it there yet, but a public web page describing these results and linking to a public note on the analysis will soon appear in the <a href="http://www-cdf.fnal.gov/physics/new/top/public_singletop.html">public web page of single top searches in CDF</a>.</p>
<p>UPDATE: The public web page of the analysis is <a href="http://www-cdf.fnal.gov/physics/new/top/2008/singletop/METbb/">here</a>, and a .pdf file with the public note describing the result is <a href="http://www-cdf.fnal.gov/cdfnotes/cdf9650_stop_metbb_pub_2.1fb.pdf">at this link</a>. Enjoy!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/1948/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/1948/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/1948/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/1948/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/1948/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/1948/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/1948/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/1948/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/1948/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/1948/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1948&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/01/14/single-top-seen-with-no-leptons/feed/</wfw:commentRss>
		<slash:comments>8</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/stmetjj_dil.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/stmetjj_std.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/singletop.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/stmetjj_nn1.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/stmetjj_nn2.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/stmetjj_res.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/stmetjj_vtb.jpg" medium="image" />
	</item>
		<item>
		<title>Some posts you might have missed in 2008 &#8211; part II</title>
		<link>http://dorigo.wordpress.com/2009/01/06/some-posts-you-might-have-missed-in-2008-part-ii/</link>
		<comments>http://dorigo.wordpress.com/2009/01/06/some-posts-you-might-have-missed-in-2008-part-ii/#comments</comments>
		<pubDate>Tue, 06 Jan 2009 17:04:30 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[anomalous muons]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[D0]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LHC]]></category>
		<category><![CDATA[Lubos Motl]]></category>
		<category><![CDATA[new physics]]></category>
		<category><![CDATA[PDF]]></category>
		<category><![CDATA[QCD]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[top mass]]></category>
		<category><![CDATA[top quark]]></category>
		<category><![CDATA[Z boson]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1918</guid>
		<description><![CDATA[Here is the second part of the list of useful physics posts I published on this site in 2008. As noted yesterday when I published the list for the first six months of 2008, this list does not include guest posts nor conference reports, which may be valuable but belong to a different place (and [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1918&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Here is the second part of the list of useful physics posts I published on this site in 2008. As <a href="http://dorigo.wordpress.com/2009/01/05/some-posts-you-might-have-missed-in-2008/">noted yesterday</a> when I published the list for the first six months of 2008, this list does not include guest posts nor conference reports, which may be valuable but belong to a different place (and are linked from permanent pages above). In reverse chronological order:</p>
<p><a href="http://dorigo.wordpress.com/2008/12/29/three-exquisite-exclusive-charmonium-signals/">December 29</a>: a report on the first measurement of exclusive production of charmonium states in hadron-hadron collisions, by CDF.</p>
<p><a href="http://dorigo.wordpress.com/2008/12/19/more-on-the-z-lineshape-at-lhc/"> December 19</a>: a detailed description of the effects of parton distribution functions on the production of Z bosons at the LHC, and how these effects determine the observed mass of the produced Z bosons. On the same topic, there is a maybe simpler <a href="http://dorigo.wordpress.com/2008/11/25/the-z-mass-at-a-hadron-collider/">post from November 25th</a>.</p>
<p><a href="http://dorigo.wordpress.com/2008/12/08/top-quark-mass-measured-with-neutrino-phi-weighting/">December 8</a>: description of a new technique to measure the top quark mass in dileptonic decays by CDF.</p>
<p><a href="http://dorigo.wordpress.com/2008/11/28/ridiculous-branching-fractions-nailed/">November 28</a>: a report on the measurement of extremely rare decays of B hadrons, and their implications.</p>
<p><a href="http://dorigo.wordpress.com/2008/11/19/an-appetizer-for-the-impatient-lubologist/">November 19</a>, <a href="http://dorigo.wordpress.com/2008/11/20/lubos-the-experimentalist/">November 20</a>, <a href="http://dorigo.wordpress.com/2008/11/20/lubos-motls-apology/">November 20 again </a>, <a href="http://dorigo.wordpress.com/2008/11/21/saving-a-good-text-from-a-few-mistakes/">November 21</a>, and <a href="http://dorigo.wordpress.com/2008/11/21/hats-off-to-lubos-motl/">November 21 again</a>: a five-post saga on the disagreement between Lubos Motl and yours truly on a detail on the multi-muon analysis by CDF, which becomes a endless diatriba since Lubos won&#8217;t listen to my attempts at making his brain work, and insists on his mistake. This leads to a back-and-forth between our blogs and a surprising happy ending when Motl finally apologizes for his mistake. Stuff for expert lubologists, but I could not help adding the above links to this summary. <span style="color:#ff0000;">Beware, most of the fun is in the comments threads!</span></p>
<p><a href="http://dorigo.wordpress.com/2008/11/08/some-notes-on-the-multi-muon-analysis-part-i/">November 8</a>, <a href="http://dorigo.wordpress.com/2008/11/08/some-notes-on-the-multi-muon-analysis-part-ii/">November 8 again</a>, and <a href="http://dorigo.wordpress.com/2008/11/12/some-notes-on-the-multi-muon-analysis-part-iii/">November 12</a>: a three-part discussion of the details in the surprising new measurement of anomalous multi-muon production published by CDF (whose summary is <a href="http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/"> here</a>). <strong>Warning:</strong> I intend to continue this series as I find the time, to complete the detailed description of this potentially groundbreaking study.</p>
<p><a href="http://dorigo.wordpress.com/2008/10/24/d0-bags-evidence-for-semileptonic-dibosons/">October 24</a>: the analysis by which D0 extracts evidence for diboson production using the dilepton plus dijet final state, a difficult, background-ridden signature. The same search, performed by CDF, is reported in detail in <a href="http://dorigo.wordpress.com/2008/10/13/the-hard-task-of-finding-hadronic-vector-boson-decays/">a post published on October 13</a>.</p>
<p><a href="http://dorigo.wordpress.com/2008/09/23/2fb-cdf-results-for-new-physics-search/">September 23</a>: a description of an automated global search for new physics in CDF data, and its intriguing results.</p>
<p><a href="http://dorigo.wordpress.com/2008/09/19/omega-b-the-new-baryon-nailed-by-d0/"> September 19</a>: the discovery of the <img src='http://l.wordpress.com/latex.php?latex=%5COmega_b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\Omega_b' title='\Omega_b' class='latex' /> baryon, an important find by the D0 experiment.</p>
<p><a href="http://dorigo.wordpress.com/2008/08/27/upsilon-polarization-a-surprise-from-d0/">August 27</a>: a report on the D0 measurement of the polarization of Upsilon mesons -states made up by a <img src='http://l.wordpress.com/latex.php?latex=b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='b \bar b' title='b \bar b' class='latex' /> pair- and its relevance for our understanding of QCD.</p>
<p><a href="http://dorigo.wordpress.com/2008/08/21/toward-a-23fb-w-mass-measurement/"> August 21</a>: a detailed discussion of the ingredients necessary to measure with the utmost precision the mass of the W boson at the Tevatron.</p>
<p><a href="http://dorigo.wordpress.com/2008/08/08/lambda-b-lifetime-checks-ok/">August 8</a>: the new CDF measurement of the lifetime of the <img src='http://l.wordpress.com/latex.php?latex=%5CLambda_b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\Lambda_b' title='\Lambda_b' class='latex' /> baryon, which had previously been in disagreement with theory.</p>
<p><a href="http://dorigo.wordpress.com/2008/08/07/combined-tevatron-higgs-limits-from-ichep-08/">August 7</a>: a discussion of the new cross-section limits on Higgs boson production, and the first exclusion of the 170 GeV mass, by the two Tevatron experiments.</p>
<p><a href="http://dorigo.wordpress.com/2008/07/18/do-you-remember-the-dimuon-bump/">July 18</a>: a search for narrow resonances decaying to muon pairs in CDF data excludes the tentative signal seen by CDF in Run I.</p>
<p><a href="http://dorigo.wordpress.com/2008/07/10/the-fascinating-b-quark-cross-sections/">July 10</a>: An important measurement by CDF on the correlated production of pairs of b-quark jets. This measurement is a cornerstone of the observation of anomalous multi-muon events that CDF published at the end of October 2008 (see above).</p>
<p><a href="http://dorigo.wordpress.com/2008/07/08/a-top-mass-measurement-technique-for-cms-and-atlas/">July 8</a>: a report of a new technique to measure the top quark mass which is very important for the LHC, and the results obtained on CDF data. For a similar technique of relevance to LHC, also check <a href="http://dorigo.wordpress.com/2008/10/03/another-pro-lhc-top-mass-measurement/">this other CDF measurement</a>.</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/1918/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/1918/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/1918/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/1918/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/1918/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/1918/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/1918/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/1918/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/1918/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/1918/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1918&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2009/01/06/some-posts-you-might-have-missed-in-2008-part-ii/feed/</wfw:commentRss>
		<slash:comments>2</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>
	</item>
		<item>
		<title>D0 bags evidence for semileptonic dibosons</title>
		<link>http://dorigo.wordpress.com/2008/10/24/d0-bags-evidence-for-semileptonic-dibosons/</link>
		<comments>http://dorigo.wordpress.com/2008/10/24/d0-bags-evidence-for-semileptonic-dibosons/#comments</comments>
		<pubDate>Fri, 24 Oct 2008 12:11:06 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[news]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[D0]]></category>
		<category><![CDATA[hadronic signals]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[Tevatron]]></category>
		<category><![CDATA[weak decays]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1665</guid>
		<description><![CDATA[A week ago I discussed here the recently approved analysis by which CDF shows a small hint of WW/WZ signal in their Run II data, with one W boson decaying to a lepton-neutrino pair, and the other boson (either a W or a Z) producing a pair of hadronic jets.
Such a process is very hard [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1665&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><a href="http://dorigo.wordpress.com/2008/10/13/the-hard-task-of-finding-hadronic-vector-boson-decays/">A week ago I discussed here</a> the recently approved analysis by which CDF shows a small hint of WW/WZ signal in their Run II data, with one W boson decaying to a lepton-neutrino pair, and the other boson (either a W or a Z) producing a pair of hadronic jets.</p>
<p>Such a process is very hard to put in evidence in hadronic collisions, due to the large irreducible background of events due to one leptonic W decay accompanied by QCD radiation from the initial state of the collision. In fact, despite having been sought by many in Run I, no appreciable signal had surfaced in Tevatron data either from CDF or D0.</p>
<p>Now, <strong>D0 has really bagged it</strong>. They used a more performant selection method than the one used by CDF, and were a bit more bold in their use of Monte Carlo simulations. The result is that they find a very significant excess, amounting roughly to 960 events, in a total of nearly 27,000.</p>
<p>I encourage those readers who are unfamiliar with the basics of vector boson production at hadron colliders to read the introductory part of the former post on this topic, which I linked above. Here I will avoid repeating that introduction, and concentrate instead on the analysis details.</p>
<p>D0 uses a total of 1.1 inverse femtobarns of 1.96 TeV proton-antiproton collisions, acquired during Run II of the Tevatron. The samples of data are collected by triggers selecting a signal of a high-energy electron or muon, and a further requirement that a transverse energy imbalance of 20 GeV or more is requested, thus characterizing the leptonic decay <img src='http://l.wordpress.com/latex.php?latex=W+%5Cto+l+%5Cnu_l&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='W \to l \nu_l' title='W \to l \nu_l' class='latex' /> of one vector boson. Finally, the transverse mass of the lepton-missing transverse energy  system has to be larger than 35 GeV, reducing backgrounds from non-W events.</p>
<p>[<em>The transverse mass is computed by neglecting the z-component of the particles momenta: if both particles are emitted perfectly transverse to the beam direction, transverse and total mass coincide. This is forced by the absence of a z-measurement of the neutrino momentum, since the energy imbalance it creates by escaping the detector cannot be measured along the proton-antiproton axis</em>.]</p>
<p>Besides characterizing the leptonic W decay, two jets with transverse energy above 20 GeV are required. After this selection, the data contain a non-negligible amount of non-W backgrounds, constituted by QCD multijet events where the leptonic W is a fake; but the bulk is due to W+jets production, where the jets arise from QCD radiation off the initial partons participating in the hard interaction. Several Monte Carlo samples are used to model the latter background process, while the former is handled by loosening the lepton identification criteria in the data: the looser the lepton requirement, the larger this contamination, such that for really loose electron and muon candidates the samples are almost purely due to QCD multijet events.</p>
<p>Signal and backgrounds are separated using a multivariate classifier to combine information from several kinematic variables. This is the Random Forest algorithm, which I had the <a href="http://dorigo.wordpress.com/2006/03/03/random-forests/">occasion to discuss in the past</a> (two years ago a student of mine used it to discriminate hadronic top events in a similar dataset in CDF). The Random Forest output is highest (close to one) for signal events, while backgrounds are given a value closer to zero. The result of the classification is shown below: the excess for high values of RF output are due to the diboson signal (in red the signal content estimated by the fit).</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/wzd01.jpg" alt="" width="460" height="509" /></p>
<p>A fit to the RF output provides the normalization of the signal and the background components, as shown above. Notice the blue &#8220;envelope&#8221; in part (b) of the plot: it is the systematic uncertainty due to background RF templates. Of course, the level of the blue curve is deceiving, since shape uncertainties are totally correlated among themselves; but the signal does stand out on top of it.</p>
<p>A plot of the dijet mass distribution confirms the interpretation, as shown below. The bottom part shows the data subtracted by background contributions (points with error bars), which compares well with the shape of the expected diboson contribution. D0 finds a combined WV (WW+WZ) cross section of <img src='http://l.wordpress.com/latex.php?latex=20.2+%5Cpm+1.4+%5Cpm+3.6+%5Cpm+1.2+pb&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='20.2 \pm 1.4 \pm 3.6 \pm 1.2 pb' title='20.2 \pm 1.4 \pm 3.6 \pm 1.2 pb' class='latex' />, where the first uncertainty is statistical, the second is systematic, and the third relates to the integrated luminosity uncertainty of the base of data used in the search. This compares well with the theoretical prediction of <img src='http://l.wordpress.com/latex.php?latex=%5Csigma%28WV%29%3D16.1+%5Cpm+0.9+pb&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\sigma(WV)=16.1 \pm 0.9 pb' title='\sigma(WV)=16.1 \pm 0.9 pb' class='latex' />.</p>
<p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/wzd02.jpg" alt="" width="446" height="509" /></p>
<p>In the plot above, the combined W/Z signal peaks at about 80 GeV, with a resolution of roughly 15 GeV; the background template uncertainty is again in blue, again underlining the difficulty of this measurement, which finds a signal excess exactly where the backgrounds peak.</p>
<p>One question I often hear asked in plots such as the one above is &#8220;why do W and Z boson peak at the same mass value ? They have a 10.7 GeV mass difference after all&#8221;. True, but the dijet mass resolution of the D0 detector is insufficient to tell the two signals apart, and what one observes is the combined shape. To be more precise, one should also add that the Z contribution in the plot is much smaller than the W one (about one third). Further, one should also point out that the heavy flavors produced by the Z boson will produce a underestimated Z mass reconstruction, due to the neutrinos often produced in the semileptonic decay of b- and c-quark jets. It is a fact that the <img src='http://l.wordpress.com/latex.php?latex=Z+%5Cto+b+%5Cbar+b&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='Z \to b \bar b' title='Z \to b \bar b' class='latex' /> decay will peak at about 83 GeV after calibration of generic jet response, due to that effect alone&#8230;</p>
<p>I like to let the authors point out that &#8220;This work further provides a validation of the analytical methods used in searches for Higgs bosons at the Tevatron&#8221;, as in the conclusion of <a href="http://xxx.lanl.gov/PS_cache/arxiv/pdf/0810/0810.3873v1.pdf">their paper</a>. Indeed, the advanced methodologies by which the Tevatron experiments are setting more and more stringent limits on Higgs boson production are perceived by some as a bit uncautious. Things appear to be well under control, it instead transpires, once one can demonstrate that a signal known to be there can be indeed extracted from samples which have a very small signal-to-background ratio, as is the case of all Higgs searches.</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/1665/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/1665/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/1665/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/1665/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/1665/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/1665/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/1665/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/1665/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/1665/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/1665/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1665&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2008/10/24/d0-bags-evidence-for-semileptonic-dibosons/feed/</wfw:commentRss>
		<slash:comments>5</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/wzd01.jpg" medium="image" />

		<media:content url="http://www.pd.infn.it/~dorigo/wzd02.jpg" medium="image" />
	</item>
		<item>
		<title>Where the heart beats</title>
		<link>http://dorigo.wordpress.com/2008/10/16/where-the-heart-beats/</link>
		<comments>http://dorigo.wordpress.com/2008/10/16/where-the-heart-beats/#comments</comments>
		<pubDate>Thu, 16 Oct 2008 10:28:23 +0000</pubDate>
		<dc:creator>dorigo</dc:creator>
				<category><![CDATA[personal]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[science]]></category>
		<category><![CDATA[CDF]]></category>
		<category><![CDATA[CMS]]></category>
		<category><![CDATA[HEP]]></category>
		<category><![CDATA[Higgs boson]]></category>
		<category><![CDATA[LHC]]></category>
		<category><![CDATA[Tevatron]]></category>

		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1631</guid>
		<description><![CDATA[
The picture above made the headlines today in  repubblica.it, one of the news sites I read most often. It shows a little mouse, originally intended as a meal supplied to a viper, managing to invert the food chain, killing the monster. I am stating the obvious when I say we usually rejoice when we [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1631&subd=dorigo&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><img class="alignnone" src="http://www.pd.infn.it/~dorigo/mousevssnake.jpg" alt="" width="460" height="294" /></p>
<p>The picture above made the headlines today in <a href="http://www.repubblica.it"> repubblica.it</a>, one of the news sites I read most often. It shows a little mouse, originally intended as a meal supplied to a viper, managing to invert the food chain, killing the monster. I am stating the obvious when I say we usually rejoice when we see something like that happening: we always root for the weak against the strong, especially if we feel weak ourselves -and don&#8217;t we all, in some respect ?</p>
<p>The picture had me thinking about the competition between the <a href="http://www-bdnew.fnal.gov/tevatron/"> Tevatron </a> and <a href="http://it.wikipedia.org/wiki/Large_Hadron_Collider">LHC</a> particle accelerators. Since the LHC has not produced a single proton-proton collision in the core of the CMS and Atlas detectors yet, while the Tevatron has supplied CDF and D0 with an <a href="http://www.fnal.gov/pub/now/tevlum.html">enormous amount of collisions</a> which are fruiting <a href="http://www-d0.fnal.gov/Run2Physics/WWW/results.htm">scores</a> of <a href="http://www-cdf.fnal.gov/physics/physics.html">groundbreaking</a> physical results, the two machines might be argued to not be competing yet. But that would be a myopic assessment, on several levels.</p>
<ul>
<li>There is competition for the funding of experiments. Lab directors, experiment heads, and faculty members are very sensitive to this issue of course, since it affects their chances of leadership and power. Funds to particle physics experiments are getting cut these days, and the many experiments have to fight against each other to keep their budget plans intact. The LHC has been competing for funding with the rest of the HEP facilities since the start of its construction, or arguably even before then.</li>
</ul>
<ul>
<li>Then there is of course the fight for a place under the media spotlights. It is a level of competition tightly connected with the funding one, but it has some additional branches, since the media attention can be an important fuel to boost the career of scientists. The recent <a href="http://dorigo.wordpress.com/2008/09/10/cern-under-siege/">media hype</a> for the startup of LHC on September 10 was a masterful organization by CERN general director Aymar, and the following <a href="http://www.math.columbia.edu/~woit/wordpress/?p=935">incident with the magnets</a> in sector 34 was troublesome to CERN as much for its media impact as it was for the lab schedule. Of course, at the Tevatron and elsewhere many met the global interest for LHC in the former occasion with ill-concealed jealousy, and the latter with more evident satisfaction.</li>
</ul>
<ul>
<li>A third level of competition, in turn somewhat connected to the second, has its ground on the scientific conferences around the world which are now scheduled every second week. Presenting scientific results at conferences is a very important item in the construction of a strong curriculum, and some talks increase the prestige of the speakers. The Tevatron has had a large share of talks allotted at all the major conferences in the recent past, due to the mass of new results it produced; but Atlas and CMS have started being allotted several talks already, which will be used to discuss &#8220;Monte Carlo analyses&#8221; rather than results on real data. Still, this causes a compression of the benefits of the Fermilab scientists.</li>
</ul>
<ul>
<li>And then there is the fight for the Higgs. The Tevatron experiments are still caressing hopes to find the Higgs boson before LHC does, and are thus squeezing their brains to improve the already excellent analyses they have been producing. This year, for the first time, a <a href="http://dorigo.wordpress.com/2008/08/07/combined-tevatron-higgs-limits-from-ichep-08/">direct limit on the Higgs boson mass</a> has been set by CDF and D0 in a joint effort. Although the limit is not stringent yet (a single mass value has been excluded, 170 GeV), the two experiments are working to wipe off the board the whole high-mass region, where the LHC would have no trouble in finding a significant signal with one year worth of data. If the Higgs is proven to be lighter than 130 GeV or so, the fight between the two sides of the Atlantic is promised to become red-hot in the next two-three years, depending on whether the Tevatron gets funded to run for the fiscal year 2010.</li>
</ul>
<ul>
<li>Finally, there might be new physics out there, and it might still be at reach of the Tevatron. The six-months delay of the LHC data taking is making this race even more interesting, especially since CDF and D0 are reaching a level of sensitivity in the SUSY parameter space that might enable them to discover new physics before LHC.</li>
</ul>
<p>So, as you see, there <em>is </em>competition in HEP between LHC and the Tevatron even if the former has not begun taking data yet. The mouse of the picture above, in my mind, is the Tevatron biting the LHC&#8217;s throat, turning the tables when everybody expects the latter to entertain itself with a quiet meal. This is still possible. If CDF or D0 discovered SUSY, such an event would be a defeat of incredible proportions for CERN, echoing the disasters of the sixties and the seventies, when the US were banqueting lavishly with new discoveries, barely leaving bread crumbs for Europe.</p>
<p>&#8220;<span style="color:#ff0000;">And where do you stand</span>&#8220;, you might well ask, since I am working for both CMS at CERN and CDF at the Tevatron ? Well, I am slightly embarassed to answer, but I must say that until CDF closes down, my heart beats for it. The first love is the one you never forget, and to that piece of rethorics today I can add the image of the little mouse. Curious feeling: I am spending 80% of my research time doing my best to help make CMS a success, but I still caress some hope that it will, at least to some extent, fail to the hands of my former love. If you think that is despicable, please consider: what is important is not who gets a Nobel prize here. It is a win-win situation for whom, like me and most of you, only cares for the advancement of science. CMS, Atlas, CDF, D0: who cares ? All I care is to find out the truth!</p>
  <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/dorigo.wordpress.com/1631/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/dorigo.wordpress.com/1631/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/dorigo.wordpress.com/1631/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/dorigo.wordpress.com/1631/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/dorigo.wordpress.com/1631/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/dorigo.wordpress.com/1631/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/dorigo.wordpress.com/1631/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/dorigo.wordpress.com/1631/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/dorigo.wordpress.com/1631/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/dorigo.wordpress.com/1631/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=dorigo.wordpress.com&blog=74297&post=1631&subd=dorigo&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://dorigo.wordpress.com/2008/10/16/where-the-heart-beats/feed/</wfw:commentRss>
		<slash:comments>6</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/23529d11d1eea8aa6e35c210d61e0cb9?s=96&#38;d=identicon&#38;r=G" medium="image">
			<media:title type="html">dorigo</media:title>
		</media:content>

		<media:content url="http://www.pd.infn.it/~dorigo/mousevssnake.jpg" medium="image" />
	</item>
	</channel>
</rss>