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	<title>Comments on: CDF publishes multi-muons!!!!</title>
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	<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/</link>
	<description>private thoughts of a physicist and chessplayer</description>
	<lastBuildDate>Thu, 24 Dec 2009 08:50:26 +0000</lastBuildDate>
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		<item>
		<title>By: apedIania</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-117320</link>
		<dc:creator>apedIania</dc:creator>
		<pubDate>Wed, 25 Nov 2009 16:57:08 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-117320</guid>
		<description>industry&#039;s love-in with 
Mr Obama frequently denounced the influence , in response to specific requests  during the campaign.  House insisted . is a long way from fruition,  George Lazenby,  Download Full-lenght Movie Review:  . with some characters  DVD DivX iPod movie , Movie online Revie: . Full-lenght DVD Hi-Def DivX quality  dined  him to push . Hi-Def iPod quality  Full Movie Review: , was released late on Friday, and icier killer Bond by 20 years),  . http://99minutes.net/?person=59446 , president&#039;s fiery former  Watch movie DVD DivX iPod movie . buzz surrounding the  Eastwood  and in his own opinion, . has been given an exclusive first  of all visitors -  Online movie Hi-Def quality .</description>
		<content:encoded><![CDATA[<p>industry&#8217;s love-in with<br />
Mr Obama frequently denounced the influence , in response to specific requests  during the campaign.  House insisted . is a long way from fruition,  George Lazenby,  Download Full-lenght Movie Review:  . with some characters  DVD DivX iPod movie , Movie online Revie: . Full-lenght DVD Hi-Def DivX quality  dined  him to push . Hi-Def iPod quality  Full Movie Review: , was released late on Friday, and icier killer Bond by 20 years),  . <a href="http://99minutes.net/?person=59446" rel="nofollow">http://99minutes.net/?person=59446</a> , president&#8217;s fiery former  Watch movie DVD DivX iPod movie . buzz surrounding the  Eastwood  and in his own opinion, . has been given an exclusive first  of all visitors &#8211;  Online movie Hi-Def quality .</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: EnjoyMedia</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-106446</link>
		<dc:creator>EnjoyMedia</dc:creator>
		<pubDate>Tue, 17 Mar 2009 16:40:40 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-106446</guid>
		<description>Nice post.</description>
		<content:encoded><![CDATA[<p>Nice post.</p>
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	<item>
		<title>By: That crazy leptonic sector: multi-muon model-making &#171; High Energy PhDs</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-104672</link>
		<dc:creator>That crazy leptonic sector: multi-muon model-making &#171; High Energy PhDs</dc:creator>
		<pubDate>Mon, 16 Feb 2009 16:44:28 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-104672</guid>
		<description>[...] the best `armchair&#8217; reading on the multi-muon anomaly is still Tommaso&#8217;s set of notes: part 0, part 1, part 2, part 3, part 4. An excellent theory-side discussion can be found at [...]</description>
		<content:encoded><![CDATA[<p>[...] the best `armchair&#8217; reading on the multi-muon anomaly is still Tommaso&#8217;s set of notes: part 0, part 1, part 2, part 3, part 4. An excellent theory-side discussion can be found at [...]</p>
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	</item>
	<item>
		<title>By: dorigo</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-103972</link>
		<dc:creator>dorigo</dc:creator>
		<pubDate>Wed, 21 Jan 2009 07:47:00 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-103972</guid>
		<description>Hi Shantanu,

I know Janet well, and she is a sort of taliban of neutrinos ;-) Seriously, she would have been my first choice had one asked me to name somebody who thought that neutrino masses were evidence of BSM physics. But things are not as simple as she paints them. The SM is still there, and as I said somewhere in this blog already (&lt;a href=&quot;http://dorigo.wordpress.com/2007/02/11/the-say-of-the-week-25/&quot; rel=&quot;nofollow&quot;&gt;here&lt;/a&gt;), 

&lt;em&gt;“The neutrino masses force an extension of the Standard Model more or less as revolutionary as a rearrangement of the furniture in the kids’ room forced by the arrival of a new baby.“ &lt;/em&gt;

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>Hi Shantanu,</p>
<p>I know Janet well, and she is a sort of taliban of neutrinos <img src='http://s.wordpress.com/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' />  Seriously, she would have been my first choice had one asked me to name somebody who thought that neutrino masses were evidence of BSM physics. But things are not as simple as she paints them. The SM is still there, and as I said somewhere in this blog already (<a href="http://dorigo.wordpress.com/2007/02/11/the-say-of-the-week-25/" rel="nofollow">here</a>), </p>
<p><em>“The neutrino masses force an extension of the Standard Model more or less as revolutionary as a rearrangement of the furniture in the kids’ room forced by the arrival of a new baby.“ </em></p>
<p>Cheers,<br />
T.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Shantanu</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-103968</link>
		<dc:creator>Shantanu</dc:creator>
		<pubDate>Wed, 21 Jan 2009 03:06:47 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-103968</guid>
		<description>Coming back to the question whether neutrino mass is evidence for physics beyond standard model, please see the abstract of this lecture
series at MIT
http://student.mit.edu/searchiap/iap-9134.html
by J. Conrad.

&quot;Neutrinos vs. the Standard Model: Because Goliath Lost!&quot;
Prof. Janet Conrad
Over years, physicists developed a &quot;Standard Model&quot; of particle physics which describes the data very well. It correctly predicted the results of nearly all particle physics experiments. Now we think the tiniest matter particle, the neutrino, shows a chink in the Standard model. This talk describes the discovery of neutrino mass and discusses the next steps in neutrino physics world-wide and at LNS.</description>
		<content:encoded><![CDATA[<p>Coming back to the question whether neutrino mass is evidence for physics beyond standard model, please see the abstract of this lecture<br />
series at MIT<br />
<a href="http://student.mit.edu/searchiap/iap-9134.html" rel="nofollow">http://student.mit.edu/searchiap/iap-9134.html</a><br />
by J. Conrad.</p>
<p>&#8220;Neutrinos vs. the Standard Model: Because Goliath Lost!&#8221;<br />
Prof. Janet Conrad<br />
Over years, physicists developed a &#8220;Standard Model&#8221; of particle physics which describes the data very well. It correctly predicted the results of nearly all particle physics experiments. Now we think the tiniest matter particle, the neutrino, shows a chink in the Standard model. This talk describes the discovery of neutrino mass and discusses the next steps in neutrino physics world-wide and at LNS.</p>
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		<title>By: Yet another leptonic excess. (MiniBooNE) &#171; High Energy PhDs</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102733</link>
		<dc:creator>Yet another leptonic excess. (MiniBooNE) &#171; High Energy PhDs</dc:creator>
		<pubDate>Mon, 15 Dec 2008 10:07:51 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102733</guid>
		<description>[...] us a speculative &#8220;multi-muon anomaly&#8221; at CDF (arXiv:0810.5357, see also Tommaso&#8217;s summary), the publication of the PAMELA cosmic-ray positron excess (arXiv:0810.4995, ), and related [...]</description>
		<content:encoded><![CDATA[<p>[...] us a speculative &#8220;multi-muon anomaly&#8221; at CDF (arXiv:0810.5357, see also Tommaso&#8217;s summary), the publication of the PAMELA cosmic-ray positron excess (arXiv:0810.4995, ), and related [...]</p>
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	<item>
		<title>By: A chat with Arkani-Hamed at CERN &#171; A Quantum Diaries Survivor</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102582</link>
		<dc:creator>A chat with Arkani-Hamed at CERN &#171; A Quantum Diaries Survivor</dc:creator>
		<pubDate>Tue, 09 Dec 2008 21:42:21 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102582</guid>
		<description>[...] This caused arguments -better call them exchanges- with Neal Weiner and with Nima Arkani-Hamed (see here for the original epistolary). Nima, in particular, had a remarkable incipit in his comment to my [...]</description>
		<content:encoded><![CDATA[<p>[...] This caused arguments -better call them exchanges- with Neal Weiner and with Nima Arkani-Hamed (see here for the original epistolary). Nima, in particular, had a remarkable incipit in his comment to my [...]</p>
]]></content:encoded>
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		<title>By: The whisper of the universe &#171; The Gauge Connection</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102410</link>
		<dc:creator>The whisper of the universe &#171; The Gauge Connection</dc:creator>
		<pubDate>Mon, 01 Dec 2008 14:41:57 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102410</guid>
		<description>[...] for too long. Whoever is interested about the relevant discussions about I just point you to the Dorigo&#8217;s blog being him one of the authors of the CDF&#8217;s paper. This provoked a lot of rumors in the [...]</description>
		<content:encoded><![CDATA[<p>[...] for too long. Whoever is interested about the relevant discussions about I just point you to the Dorigo&#8217;s blog being him one of the authors of the CDF&#8217;s paper. This provoked a lot of rumors in the [...]</p>
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		<title>By: dorigo</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102264</link>
		<dc:creator>dorigo</dc:creator>
		<pubDate>Mon, 24 Nov 2008 19:46:17 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102264</guid>
		<description>... To clarify: if there is a bug in GEANT, it might affect both detectors equally. If Fermilab received a batch of iron which is iron-plated aluminum, both detectors have less material than they expect, and more muon fakes. There are dozens of ways a correlation may exist between the counting of muons in D0 and CDF... All quite improbable, but if compared to the new physics we are talking about... Well...

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>&#8230; To clarify: if there is a bug in GEANT, it might affect both detectors equally. If Fermilab received a batch of iron which is iron-plated aluminum, both detectors have less material than they expect, and more muon fakes. There are dozens of ways a correlation may exist between the counting of muons in D0 and CDF&#8230; All quite improbable, but if compared to the new physics we are talking about&#8230; Well&#8230;</p>
<p>Cheers,<br />
T.</p>
]]></content:encoded>
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	<item>
		<title>By: dorigo</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102263</link>
		<dc:creator>dorigo</dc:creator>
		<pubDate>Mon, 24 Nov 2008 19:44:25 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102263</guid>
		<description>Hi Elias,

I think the D0 measurement is 2.3+-0.7, not 2.6. 
In a sense, yes, it is an indication that D0, were to do the same analysis, would probably find some excess too. However, while CDF has measured the bb xs with both SVX and dimuons, D0 has done it only with dimuons. If D0 found a number close to NLO with secondary vertices, that alone would be some indication that they too have a unknown extra source of muons. 

Whether that is new physics or some screwup in the simulation of energy loss and other effects in the material, is not granted though.

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>Hi Elias,</p>
<p>I think the D0 measurement is 2.3+-0.7, not 2.6.<br />
In a sense, yes, it is an indication that D0, were to do the same analysis, would probably find some excess too. However, while CDF has measured the bb xs with both SVX and dimuons, D0 has done it only with dimuons. If D0 found a number close to NLO with secondary vertices, that alone would be some indication that they too have a unknown extra source of muons. </p>
<p>Whether that is new physics or some screwup in the simulation of energy loss and other effects in the material, is not granted though.</p>
<p>Cheers,<br />
T.</p>
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		<title>By: Elias Lopez</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102262</link>
		<dc:creator>Elias Lopez</dc:creator>
		<pubDate>Mon, 24 Nov 2008 18:51:42 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102262</guid>
		<description>Hi Tommaso,

I have a question:
As far as I know, one of the motivations that led to the observation of this unexpectedly large sample of events with muons at CDF was the measurement of discrepant bb cross sections (I mean, discrepant with respect to the SM predictions).
In the paper by the CDF collaboration published in Phys. Rev. D 77, with reference 072004 (the one in that the &quot;tight SVT cuts&quot; are applied), I read that not only CDF reported a measurement of R2b (the ratio of the measured bb cross section to the exact NLO prediction) unexpectedly large (3.0+/-0.6), but also D0 (2.6+/-0.7).
As I understand (according to the paper just released by CDF), the origin of this value of R2b (at CDF) are the &quot;ghost muons&quot; that in a posterior analysis are cutted by the &quot;tight SVT cuts&quot;. And my question is: Does the fact that there has been another (independent, I supose) measurement of R2b at D0 consistent with the one obtained by CDF support the idea that the observed &quot;ghost muon sample&quot; is really new physics, and not a failure in the analysis?
Thank you very much,

Elías</description>
		<content:encoded><![CDATA[<p>Hi Tommaso,</p>
<p>I have a question:<br />
As far as I know, one of the motivations that led to the observation of this unexpectedly large sample of events with muons at CDF was the measurement of discrepant bb cross sections (I mean, discrepant with respect to the SM predictions).<br />
In the paper by the CDF collaboration published in Phys. Rev. D 77, with reference 072004 (the one in that the &#8220;tight SVT cuts&#8221; are applied), I read that not only CDF reported a measurement of R2b (the ratio of the measured bb cross section to the exact NLO prediction) unexpectedly large (3.0+/-0.6), but also D0 (2.6+/-0.7).<br />
As I understand (according to the paper just released by CDF), the origin of this value of R2b (at CDF) are the &#8220;ghost muons&#8221; that in a posterior analysis are cutted by the &#8220;tight SVT cuts&#8221;. And my question is: Does the fact that there has been another (independent, I supose) measurement of R2b at D0 consistent with the one obtained by CDF support the idea that the observed &#8220;ghost muon sample&#8221; is really new physics, and not a failure in the analysis?<br />
Thank you very much,</p>
<p>Elías</p>
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	<item>
		<title>By: dorigo</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102091</link>
		<dc:creator>dorigo</dc:creator>
		<pubDate>Thu, 20 Nov 2008 07:04:03 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102091</guid>
		<description>Dear Wouter,

as far as your second question is concerned, I can answer it straight away: although not a rigorous procedure, the tail of the impact parameter distribution can be fit with $latex f(d_0)=k \exp^{(-d_0/c \tau)}$, extracting the particle&#039;s $latex c \tau$ with good precision, regardless of the particle&#039;s momentum spectrum. That is because the impact parameter remains invariant for lorentz boosts: the larger the $latex \beta \gamma$, the longer the particle travels (by a distance $latex L=\beta \gamma c \tau$), and d scales accordingly.

As for your first question, I have an answer for you, but I prefer to check it with the author of the analysis, because there might be a subtlety and I do not want to mislead you, given that you will be making use of the information. I will get back to you shortly on that.

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>Dear Wouter,</p>
<p>as far as your second question is concerned, I can answer it straight away: although not a rigorous procedure, the tail of the impact parameter distribution can be fit with <img src='http://l.wordpress.com/latex.php?latex=f%28d_0%29%3Dk+%5Cexp%5E%7B%28-d_0%2Fc+%5Ctau%29%7D&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='f(d_0)=k \exp^{(-d_0/c \tau)}' title='f(d_0)=k \exp^{(-d_0/c \tau)}' class='latex' />, extracting the particle&#8217;s <img src='http://l.wordpress.com/latex.php?latex=c+%5Ctau&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='c \tau' title='c \tau' class='latex' /> with good precision, regardless of the particle&#8217;s momentum spectrum. That is because the impact parameter remains invariant for lorentz boosts: the larger the <img src='http://l.wordpress.com/latex.php?latex=%5Cbeta+%5Cgamma&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='\beta \gamma' title='\beta \gamma' class='latex' />, the longer the particle travels (by a distance <img src='http://l.wordpress.com/latex.php?latex=L%3D%5Cbeta+%5Cgamma+c+%5Ctau&#038;bg=ffffff&#038;fg=000000&#038;s=0' alt='L=\beta \gamma c \tau' title='L=\beta \gamma c \tau' class='latex' />), and d scales accordingly.</p>
<p>As for your first question, I have an answer for you, but I prefer to check it with the author of the analysis, because there might be a subtlety and I do not want to mislead you, given that you will be making use of the information. I will get back to you shortly on that.</p>
<p>Cheers,<br />
T.</p>
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		<title>By: Cullen T.M. McGough</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102086</link>
		<dc:creator>Cullen T.M. McGough</dc:creator>
		<pubDate>Thu, 20 Nov 2008 02:56:42 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102086</guid>
		<description>Oh, lookie there. The icons are auto-magic. How nice.</description>
		<content:encoded><![CDATA[<p>Oh, lookie there. The icons are auto-magic. How nice.</p>
]]></content:encoded>
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	<item>
		<title>By: Cullen T.M. McGough</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102085</link>
		<dc:creator>Cullen T.M. McGough</dc:creator>
		<pubDate>Thu, 20 Nov 2008 02:55:24 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102085</guid>
		<description>Ok, sorry to interrupt the serious discussion, but I&#039;m irritated.

I was reading Neal Stephenson&#039;s new book and he mentions &quot;quantum cross-talk&quot; as a mechanism for the transfer of data between discrete cosmi in a polycosmic interpretation of the universe. 

I happen to look up at a stupid poster of moon phases on the wall, and realize that if such a thing actually existed, higher density regions (like neutron stars) would have the greatest cross-talk. So I google &quot;quantum cross talk&quot; and get this blog. 

Now. I only understand every 6th word you guys are babbling on about, but you seem to be talking about verified (sort of) tests that witness extra muons popping into this cosmos without source?

And, to make it worse, 80% of you are using avatar icons representing tiling problems, just like Stephenson&#039;s obsessive polycosmos &quot;Lineage&quot; cult dudes.

Damn it, damn it.

Please try to avoid collapsing this cosmos into a singularity.</description>
		<content:encoded><![CDATA[<p>Ok, sorry to interrupt the serious discussion, but I&#8217;m irritated.</p>
<p>I was reading Neal Stephenson&#8217;s new book and he mentions &#8220;quantum cross-talk&#8221; as a mechanism for the transfer of data between discrete cosmi in a polycosmic interpretation of the universe. </p>
<p>I happen to look up at a stupid poster of moon phases on the wall, and realize that if such a thing actually existed, higher density regions (like neutron stars) would have the greatest cross-talk. So I google &#8220;quantum cross talk&#8221; and get this blog. </p>
<p>Now. I only understand every 6th word you guys are babbling on about, but you seem to be talking about verified (sort of) tests that witness extra muons popping into this cosmos without source?</p>
<p>And, to make it worse, 80% of you are using avatar icons representing tiling problems, just like Stephenson&#8217;s obsessive polycosmos &#8220;Lineage&#8221; cult dudes.</p>
<p>Damn it, damn it.</p>
<p>Please try to avoid collapsing this cosmos into a singularity.</p>
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	<item>
		<title>By: Wouter Hulsbergen</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102074</link>
		<dc:creator>Wouter Hulsbergen</dc:creator>
		<pubDate>Wed, 19 Nov 2008 21:37:24 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102074</guid>
		<description>Hi Tomasso,

I am trying to digest the paper for a discussion in our group in A&#039;dam and I have two burning questions: 
- How is the QCD contribution subtracted to obtain the &#039;ghost&#039; distribution for muon impact parameters in figure 7 (the first figure above)? And for example for the D0 invariant mass in figure 4?
- To obtain a lifetime from the distributions in figure 26 (last pictures shown above), you&#039;ll need a momentum measurement. How is the momentum of these candidates estimated? This is not described in the paper.

Thanks a lot,
Wouter</description>
		<content:encoded><![CDATA[<p>Hi Tomasso,</p>
<p>I am trying to digest the paper for a discussion in our group in A&#8217;dam and I have two burning questions:<br />
- How is the QCD contribution subtracted to obtain the &#8216;ghost&#8217; distribution for muon impact parameters in figure 7 (the first figure above)? And for example for the D0 invariant mass in figure 4?<br />
- To obtain a lifetime from the distributions in figure 26 (last pictures shown above), you&#8217;ll need a momentum measurement. How is the momentum of these candidates estimated? This is not described in the paper.</p>
<p>Thanks a lot,<br />
Wouter</p>
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		<title>By: An appetizer for the impatient lubologist &#171; A Quantum Diaries Survivor</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-102071</link>
		<dc:creator>An appetizer for the impatient lubologist &#171; A Quantum Diaries Survivor</dc:creator>
		<pubDate>Wed, 19 Nov 2008 20:45:14 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-102071</guid>
		<description>[...] explaining why Strassler&#8217;s estimate of the cross section of &#8220;ghost events&#8221; in the recent CDF publication is right, and I am [...]</description>
		<content:encoded><![CDATA[<p>[...] explaining why Strassler&#8217;s estimate of the cross section of &#8220;ghost events&#8221; in the recent CDF publication is right, and I am [...]</p>
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		<title>By: Like Stepping Into a Whole Different Intartube &#124; Screaming Planet</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-101897</link>
		<dc:creator>Like Stepping Into a Whole Different Intartube &#124; Screaming Planet</dc:creator>
		<pubDate>Mon, 10 Nov 2008 14:13:34 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-101897</guid>
		<description>[...] subjects to comment on something entirely bizarre. While browsing the web, I ran across this blog post. Reading the page, I started feeling a mounting sense of unease about the contents. Not about the [...]</description>
		<content:encoded><![CDATA[<p>[...] subjects to comment on something entirely bizarre. While browsing the web, I ran across this blog post. Reading the page, I started feeling a mounting sense of unease about the contents. Not about the [...]</p>
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		<title>By: Hello world! &#171; How the World Works</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-101890</link>
		<dc:creator>Hello world! &#171; How the World Works</dc:creator>
		<pubDate>Mon, 10 Nov 2008 01:40:11 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-101890</guid>
		<description>[...] Here is more detail from one of the experimenters: CDF publishes multi-muons!!!! [...]</description>
		<content:encoded><![CDATA[<p>[...] Here is more detail from one of the experimenters: CDF publishes multi-muons!!!! [...]</p>
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		<title>By: Alejandro Rivero</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-101838</link>
		<dc:creator>Alejandro Rivero</dc:creator>
		<pubDate>Fri, 07 Nov 2008 14:18:33 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-101838</guid>
		<description>(a remark about my #39 above: great part of the stability of B decays comes really from its CKM term; this is not seen explicitly in the plots)</description>
		<content:encoded><![CDATA[<p>(a remark about my #39 above: great part of the stability of B decays comes really from its CKM term; this is not seen explicitly in the plots)</p>
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		<title>By: erhard seiler</title>
		<link>http://dorigo.wordpress.com/2008/10/31/cdf-publishes-multi-muons/#comment-101802</link>
		<dc:creator>erhard seiler</dc:creator>
		<pubDate>Wed, 05 Nov 2008 14:08:25 +0000</pubDate>
		<guid isPermaLink="false">http://dorigo.wordpress.com/?p=1678#comment-101802</guid>
		<description>read this!</description>
		<content:encoded><![CDATA[<p>read this!</p>
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