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	<title>Comments on: The LHC Dashboard</title>
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	<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/</link>
	<description>Random samplings from a universe of ideas.</description>
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	<item>
		<title>By: Thanksgiving &#124; Cosmic Variance &#124; Discover Magazine</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-49650</link>
		<dc:creator>Thanksgiving &#124; Cosmic Variance &#124; Discover Magazine</dc:creator>
		<pubDate>Thu, 27 Nov 2008 16:52:21 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-49650</guid>
		<description>[...] every challenge that particle accelerators could think to throw at it. But it&#8217;s going to be blown out of the water in a couple of years. Still, a pretty good run. Thanks, Standard Model [...]</description>
		<content:encoded><![CDATA[<p>[...] every challenge that particle accelerators could think to throw at it. But it&#8217;s going to be blown out of the water in a couple of years. Still, a pretty good run. Thanks, Standard Model [...]</p>
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	<item>
		<title>By: The Big Bang Experiment - Page 5 - Meez Forums</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17954</link>
		<dc:creator>The Big Bang Experiment - Page 5 - Meez Forums</dc:creator>
		<pubDate>Sat, 13 Sep 2008 15:57:09 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17954</guid>
		<description>[...] to an old Cosmic Variance post, the power of one of the LHC&#039;s proton beams at full energy is 10 trillion watts (TW). (A watt is a [...]</description>
		<content:encoded><![CDATA[<p>[...] to an old Cosmic Variance post, the power of one of the LHC&#8217;s proton beams at full energy is 10 trillion watts (TW). (A watt is a [...]</p>
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	</item>
	<item>
		<title>By: Will CERN Destroy The World? &#171; ab initio. ab intra.</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17953</link>
		<dc:creator>Will CERN Destroy The World? &#171; ab initio. ab intra.</dc:creator>
		<pubDate>Sat, 02 Aug 2008 19:04:00 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17953</guid>
		<description>[...] LHC startup plan. Includes dates, energies and luminosities [...]</description>
		<content:encoded><![CDATA[<p>[...] LHC startup plan. Includes dates, energies and luminosities [...]</p>
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	</item>
	<item>
		<title>By: LHC dates</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17952</link>
		<dc:creator>LHC dates</dc:creator>
		<pubDate>Sat, 31 Mar 2007 21:47:09 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17952</guid>
		<description>[...] So here it is: http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/ [...]</description>
		<content:encoded><![CDATA[<p>[...] So here it is: <a href="http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/" rel="nofollow">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/</a> [...]</p>
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	</item>
	<item>
		<title>By: Thanksgiving &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17951</link>
		<dc:creator>Thanksgiving &#124; Cosmic Variance</dc:creator>
		<pubDate>Thu, 23 Nov 2006 18:26:41 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17951</guid>
		<description>[...] It&#8217;s served us well for three decades, withstanding every challenge that particle accelerators could think to throw at it. But it&#8217;s going to be blown out of the water in a couple of years. Still, a pretty good run. Thanks, Standard Model Lagrangian! [...]</description>
		<content:encoded><![CDATA[<p>[...] It&#8217;s served us well for three decades, withstanding every challenge that particle accelerators could think to throw at it. But it&#8217;s going to be blown out of the water in a couple of years. Still, a pretty good run. Thanks, Standard Model Lagrangian! [...]</p>
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	</item>
	<item>
		<title>By: End of the summer school season &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17927</link>
		<dc:creator>End of the summer school season &#124; Cosmic Variance</dc:creator>
		<pubDate>Mon, 18 Sep 2006 22:28:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17927</guid>
		<description>[...] Hey, Lufthansa has wireless in the sky â€&quot; how cool is that! So here I am at roughly 38,000 ft, somewhere over Canada, 6.5 hours into the flight with 4.5 hours left to go.... I&#039;m on my way home from the International Center for Theoretical Physics (ICTP) in Trieste, Italy, where one of the last summer schools of the season just finished. The topic was Expecting LHC, which was the hot topic for summer schools this year. In fact, everybody who is anybody had one. The LHC is turning on next year and everyone wants the new crop of graduate students to be prepared! [...]</description>
		<content:encoded><![CDATA[<p>[...] Hey, Lufthansa has wireless in the sky â€&#8221; how cool is that! So here I am at roughly 38,000 ft, somewhere over Canada, 6.5 hours into the flight with 4.5 hours left to go&#8230;. I&#8217;m on my way home from the International Center for Theoretical Physics (ICTP) in Trieste, Italy, where one of the last summer schools of the season just finished. The topic was Expecting LHC, which was the hot topic for summer schools this year. In fact, everybody who is anybody had one. The LHC is turning on next year and everyone wants the new crop of graduate students to be prepared! [...]</p>
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	</item>
	<item>
		<title>By: Life as a Physicist &#187; 1 pb-1</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17926</link>
		<dc:creator>Life as a Physicist &#187; 1 pb-1</dc:creator>
		<pubDate>Thu, 29 Jun 2006 08:29:10 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17926</guid>
		<description>[...] The reasons for the delay are varied. As pointed out over on Cosmic Variance, the main problem is not enough of the magnets will be commissioned and certified to run at the currents required to bend a 7 TeV beam of protons. It would be foolish to push them further before you carefully test them. In a system this large and complex is pays in the long run to do it bit-by-bit no matter how frustrating. [...]</description>
		<content:encoded><![CDATA[<p>[...] The reasons for the delay are varied. As pointed out over on Cosmic Variance, the main problem is not enough of the magnets will be commissioned and certified to run at the currents required to bend a 7 TeV beam of protons. It would be foolish to push them further before you carefully test them. In a system this large and complex is pays in the long run to do it bit-by-bit no matter how frustrating. [...]</p>
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	</item>
	<item>
		<title>By: The Story So Far&#8230; &#187; Blog Archive &#187; While Probing The Fabric Of The Universe, Wear Your Safety Goggles</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17950</link>
		<dc:creator>The Story So Far&#8230; &#187; Blog Archive &#187; While Probing The Fabric Of The Universe, Wear Your Safety Goggles</dc:creator>
		<pubDate>Fri, 23 Jun 2006 20:24:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17950</guid>
		<description>[...] But they need to be a tad careful in turning it on...&#160; [...]</description>
		<content:encoded><![CDATA[<p>[...] But they need to be a tad careful in turning it on&#8230;&nbsp; [...]</p>
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	<item>
		<title>By: JoAnne</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17925</link>
		<dc:creator>JoAnne</dc:creator>
		<pubDate>Fri, 23 Jun 2006 05:29:10 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17925</guid>
		<description>Peter,

As a fellow blogger I see you understand that the likelihood of getting your question anwered is directly correlated to the niceness of your comment!

Seriously, I saw this on your blog yesterday and meant to respond but got distracted.  I am glad you brought it up again.

So, regarding when announcements of discoveries will come out of the LHC - it depends, naturally, on what is being discovered.  If there really are blackholes at a TeV, or if there is a heavy gauge boson (or Randall-Sundrum type graviton Kaluza-Klein resonances) at 2-3 TeV, then we will know very quickly.  Probably during the 2008 physics run.  However, missing energy signatures (such as for Supersymmetry) or the Higgs to gamma gamma channel will take a few YEARS.  Those signatures require exact calibration and knowledge of the detector.

Now, you asked about the LHC Olympics.  Up to this point, this excerise has been largely ignored by the phenomenological community, because quite frankly we find it rather useless.  This excerise is precisely what our research has been about for the last 20 years and we feel that we don&#039;t need to bone up on the basics.  However, part of the more formal particle and string community have been working on it.  I am not aware of any great progress, but then, I admit that I have not been paying much attention.

Joe Lykken, in his summary talk at the yearly phenomenology meeting, Pheno06, presented a quiz to the phenomenology community.  He presented two examples of possible &quot;discoveries at the LHC,&quot; the first was simply top-quark production and the second was a combination of the production of a couple of new particles.  Joe simply showed some kinematical distributions, just as any experimenter would do during a talk, and asked the audience to guess what the signal was.  The result - well, we nailed the top-quark production signal instantaneously, and after a couple of minutes got the double new particle production too.

My point, I guess, is that the LHC Olympics folks have alot of catching up to do.  I think it is good that they realize this and are interested and are working on it.</description>
		<content:encoded><![CDATA[<p>Peter,</p>
<p>As a fellow blogger I see you understand that the likelihood of getting your question anwered is directly correlated to the niceness of your comment!</p>
<p>Seriously, I saw this on your blog yesterday and meant to respond but got distracted.  I am glad you brought it up again.</p>
<p>So, regarding when announcements of discoveries will come out of the LHC &#8211; it depends, naturally, on what is being discovered.  If there really are blackholes at a TeV, or if there is a heavy gauge boson (or Randall-Sundrum type graviton Kaluza-Klein resonances) at 2-3 TeV, then we will know very quickly.  Probably during the 2008 physics run.  However, missing energy signatures (such as for Supersymmetry) or the Higgs to gamma gamma channel will take a few YEARS.  Those signatures require exact calibration and knowledge of the detector.</p>
<p>Now, you asked about the LHC Olympics.  Up to this point, this excerise has been largely ignored by the phenomenological community, because quite frankly we find it rather useless.  This excerise is precisely what our research has been about for the last 20 years and we feel that we don&#8217;t need to bone up on the basics.  However, part of the more formal particle and string community have been working on it.  I am not aware of any great progress, but then, I admit that I have not been paying much attention.</p>
<p>Joe Lykken, in his summary talk at the yearly phenomenology meeting, Pheno06, presented a quiz to the phenomenology community.  He presented two examples of possible &#8220;discoveries at the LHC,&#8221; the first was simply top-quark production and the second was a combination of the production of a couple of new particles.  Joe simply showed some kinematical distributions, just as any experimenter would do during a talk, and asked the audience to guess what the signal was.  The result &#8211; well, we nailed the top-quark production signal instantaneously, and after a couple of minutes got the double new particle production too.</p>
<p>My point, I guess, is that the LHC Olympics folks have alot of catching up to do.  I think it is good that they realize this and are interested and are working on it.</p>
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		<title>By: Peter Woit</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17949</link>
		<dc:creator>Peter Woit</dc:creator>
		<pubDate>Thu, 22 Jun 2006 21:20:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17949</guid>
		<description>JoAnne,

Your prose is brilliant.

Tommaso Dorigo says he predicts nothing coming out before summer 2009.  When data does come out, do you think the theorists who have been participating in the &quot;LHC Olympics&quot; will be able to put what they have learned to use?</description>
		<content:encoded><![CDATA[<p>JoAnne,</p>
<p>Your prose is brilliant.</p>
<p>Tommaso Dorigo says he predicts nothing coming out before summer 2009.  When data does come out, do you think the theorists who have been participating in the &#8220;LHC Olympics&#8221; will be able to put what they have learned to use?</p>
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		<title>By: Alejandro Rivero</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17948</link>
		<dc:creator>Alejandro Rivero</dc:creator>
		<pubDate>Thu, 22 Jun 2006 21:14:56 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17948</guid>
		<description>(the daily nutritional needs, I mean)</description>
		<content:encoded><![CDATA[<p>(the daily nutritional needs, I mean)</p>
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		<title>By: Alejandro Rivero</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17947</link>
		<dc:creator>Alejandro Rivero</dc:creator>
		<pubDate>Thu, 22 Jun 2006 21:14:01 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17947</guid>
		<description>#19, Q, well, the nutritional needs of an adult human are about 2kwh, so well inside the megajoule range.</description>
		<content:encoded><![CDATA[<p>#19, Q, well, the nutritional needs of an adult human are about 2kwh, so well inside the megajoule range.</p>
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		<title>By: Count Iblis</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17946</link>
		<dc:creator>Count Iblis</dc:creator>
		<pubDate>Thu, 22 Jun 2006 13:06:40 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17946</guid>
		<description>10^(13)Watt = 4.1 x 10^(-2) GeV^2 :)</description>
		<content:encoded><![CDATA[<p>10^(13)Watt = 4.1 x 10^(-2) GeV^2 <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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		<title>By: JoAnne</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17918</link>
		<dc:creator>JoAnne</dc:creator>
		<pubDate>Wed, 21 Jun 2006 22:59:16 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17918</guid>
		<description>jls: thanks.  You have obviously learned that flattery will get you very far in this world!  I think all commenters should do nothing but praise my brilliant prose.

Garbage:  Please read my comment #24.

Tony Smith:  The subject of how/when the LHC folks are going to release their data is literally going to be the subject of my next post.  So stayed tuned....</description>
		<content:encoded><![CDATA[<p>jls: thanks.  You have obviously learned that flattery will get you very far in this world!  I think all commenters should do nothing but praise my brilliant prose.</p>
<p>Garbage:  Please read my comment #24.</p>
<p>Tony Smith:  The subject of how/when the LHC folks are going to release their data is literally going to be the subject of my next post.  So stayed tuned&#8230;.</p>
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		<title>By: garbage</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17919</link>
		<dc:creator>garbage</dc:creator>
		<pubDate>Wed, 21 Jun 2006 22:53:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17919</guid>
		<description>&quot;The energy stored in the LHC beam is 700 MegaJoules, or 10 TeraWatts. How big is that? Well, 10 TeraWatts is about half of the world&#039;s total energy output.&quot;

I&#039;m confused with the choice of units. Furthermore, are u gonna tell me that the LHC stores half the total energy output of the world!!....per century? :)</description>
		<content:encoded><![CDATA[<p>&#8220;The energy stored in the LHC beam is 700 MegaJoules, or 10 TeraWatts. How big is that? Well, 10 TeraWatts is about half of the world&#8217;s total energy output.&#8221;</p>
<p>I&#8217;m confused with the choice of units. Furthermore, are u gonna tell me that the LHC stores half the total energy output of the world!!&#8230;.per century? <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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		<title>By: jls</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17924</link>
		<dc:creator>jls</dc:creator>
		<pubDate>Wed, 21 Jun 2006 21:10:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17924</guid>
		<description>JoAnne, thanks a lot for the update and the pointer to the LHC dashboard.  I really appreciate the information and the time you spent to keep everyone posted.</description>
		<content:encoded><![CDATA[<p>JoAnne, thanks a lot for the update and the pointer to the LHC dashboard.  I really appreciate the information and the time you spent to keep everyone posted.</p>
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		<title>By: quasar9</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17922</link>
		<dc:creator>quasar9</dc:creator>
		<pubDate>Wed, 21 Jun 2006 19:07:34 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17922</guid>
		<description>JoAnne said: &quot;Sue me!&quot;
Now I definitely know it&#039;s a JoAnne gotta laugh day. lol! - Q</description>
		<content:encoded><![CDATA[<p>JoAnne said: &#8220;Sue me!&#8221;<br />
Now I definitely know it&#8217;s a JoAnne gotta laugh day. lol! &#8211; Q</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17921</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Wed, 21 Jun 2006 19:06:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17921</guid>
		<description>Oh, but JoAnne, they will sue you.  Under the Blogger&#039;s Responsibilities Omnibus Reconciliation Act of 2005, the existence of a trivial mistake in a blog post entitles readers to demand compensation to the tune of &lt;em&gt;one thousand times&lt;/em&gt; the fee they are paying to read this lovingly-constructed blog.

So be careful, willya?</description>
		<content:encoded><![CDATA[<p>Oh, but JoAnne, they will sue you.  Under the Blogger&#8217;s Responsibilities Omnibus Reconciliation Act of 2005, the existence of a trivial mistake in a blog post entitles readers to demand compensation to the tune of <em>one thousand times</em> the fee they are paying to read this lovingly-constructed blog.</p>
<p>So be careful, willya?</p>
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		<title>By: JoAnne</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17920</link>
		<dc:creator>JoAnne</dc:creator>
		<pubDate>Wed, 21 Jun 2006 18:58:44 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17920</guid>
		<description>So I forgot to give the elasped time when converting from energy to power and I used a funny capitalization.  Sue me!

The physical definition of power is the rate at which work is done, P = dE/dt.  In units, 1 Watt = 1 Joule/second.  The 10 TeraWatt figure is the power dispensed by the beam in the fraction of a second it takes to be aborted.  Given the numbers above, that fraction of a second works out to be roughly 10^-4.</description>
		<content:encoded><![CDATA[<p>So I forgot to give the elasped time when converting from energy to power and I used a funny capitalization.  Sue me!</p>
<p>The physical definition of power is the rate at which work is done, P = dE/dt.  In units, 1 Watt = 1 Joule/second.  The 10 TeraWatt figure is the power dispensed by the beam in the fraction of a second it takes to be aborted.  Given the numbers above, that fraction of a second works out to be roughly 10^-4.</p>
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		<title>By: Tony Smith</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/comment-page-1/#comment-17923</link>
		<dc:creator>Tony Smith</dc:creator>
		<pubDate>Wed, 21 Jun 2006 16:28:58 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/06/20/the-lhc-dashboard/#comment-17923</guid>
		<description>JoAnne said, about LHC, &quot;...  The plan is for full commissioning for 7 TeV beams to be completed during the winter 2008 shutdown, with the first physics run at 14 TeV center of mass energy to commence on 1 April 2008. And that&#039;s no joke.  ...&quot;.

Peter Woit asked (in a comment on his blog pingbacking this blog entry):
&quot;... Anyone want to guess how long it will be from April 2008 until the experiments have enough data to say something interesting, understand their backgrounds, and are ready to go public with results of the data analysis? How long did it take in the case of the Tevatron? ...&quot;.

In the case of the Tevatron with respect to discovery of the T-quark, here are some quotes from the book &quot;The Evidence for the Top Quark&quot; by Kent W. Staley (Cambridge 2004), with my comments [in brackets]:

&quot;... As of February 1987,CDF expected to begin their ... run in November of the same year ...

... the lab ... revised the schedule ... begin antiproton transfers to the Tevatron on June 6  1988 ... [schedule revision similar to LHC now]

Throughout the 1988-89 run, CDF was in a kind of race with ... UA2 ... at CERN ... CDF won this &quot;race&quot; early in 1989, not by finding the top, but by showing ... a top mass limit that ruled out its discovery by UA2 ... [ similar to LHC winning the Higgs race when its mass appeared to be at beyond the reach of Fermilab]

around ... 1991 ... Kondo analyzed ... the first ... published ... CDF dilepton event ... from the 1988-89 data ... Kondo found that the event could be reconstructed as the decay of a top-antitop pair, with a top mass of around 130 GeV/c^2, but &quot;it has a very broad error&quot; ... Kondo ... wanted to publish ...[a]... paper in PRL ... The paper met resistance from the collaboration, who felt it too closely resembled a top discovery claim ... Kondo &quot;didn&#039;t make ... trouble&quot;, and instead published the paper in the Journal of the Physical Society of Japan ...

In 1991 ... Goldstein and Dalitz  ... were trying to apply their method [of data analysis] to the first CDF dilepton event ...[so they]... asked ... Sliwa ... for ... help ...

Goldstein and Sliwa ... presented results at a heavy flavors group meeting in April [1992] ... showing a bump in the probability distribution at a top-quark mass of about 120 GeV/c^2 ... After that, according to Sliwa, &quot;Goldstein was told not to come to Top Group meetings,&quot; a decision that Sliwa believed was &quot;highly improper&quot; ...

the July 24 [1992] issue of Science ... described the position of Dalitz and Goldstein ... &quot;They think the patterns they found look suspiciously, though not unambiguously, like the top quark and deserve further analysis.&quot; CDF, the article noted, &quot;isn&#039;t impressed&quot; ... The Science article described Dalitz and Goldstein as having &quot;gained access to unpublished, partially analyzed CDF data only when Krys Sliwa, a member of the group, shared it without telling his colleagues.&quot; ... Goldstein denied both the sense of furtiveness and and secrecy conveyed by the Science article...

In June of 1992 ... the run designated &quot;Ia&quot; began ...

On October 29, 1992, just prior to the meeting of the ... DPF ... CDF recorded an event that looked strikingly like an e - mu top decay ... In fact, although it was not known at the time, one of the jets in this event would be tagged by both the SVX and SLT b-tagging algorithms ... some collaboration members even regarded the event by itself as worthy of publication as a top-quark event ... the event, ... known as &quot;the DPF event&quot;, would be shown at the meeting ... No claim would be made what the event signified ...

On April 26, 1994, ... CDF ... release[d] ... a paper describing &quot;evidence for top quark production&quot; ... D-zero did not claim to have established such evidence ...&quot;.

Some questions that come to mind:

1 - How will LHC deal with release of individual event data, to avoid controversies and yet permit outsiders to contribute their methods and interpretations,
in the light of the fact that the Kondo and Dalitz/Goldstein/Sliwa methods of analysis were (and still are) useful techniques developed outside the collaboration ?

2 - How will LHC deal with release of its internal analyses, bearing in mind that the DPF event was released in 1992 and it was not until 1994 that a discovery &quot;evidence&quot; paper was released ?

Tony Smith
http://www.valdostamuseum.org/hamsmith/</description>
		<content:encoded><![CDATA[<p>JoAnne said, about LHC, &#8220;&#8230;  The plan is for full commissioning for 7 TeV beams to be completed during the winter 2008 shutdown, with the first physics run at 14 TeV center of mass energy to commence on 1 April 2008. And that&#8217;s no joke.  &#8230;&#8221;.</p>
<p>Peter Woit asked (in a comment on his blog pingbacking this blog entry):<br />
&#8220;&#8230; Anyone want to guess how long it will be from April 2008 until the experiments have enough data to say something interesting, understand their backgrounds, and are ready to go public with results of the data analysis? How long did it take in the case of the Tevatron? &#8230;&#8221;.</p>
<p>In the case of the Tevatron with respect to discovery of the T-quark, here are some quotes from the book &#8220;The Evidence for the Top Quark&#8221; by Kent W. Staley (Cambridge 2004), with my comments [in brackets]:</p>
<p>&#8220;&#8230; As of February 1987,CDF expected to begin their &#8230; run in November of the same year &#8230;</p>
<p>&#8230; the lab &#8230; revised the schedule &#8230; begin antiproton transfers to the Tevatron on June 6  1988 &#8230; [schedule revision similar to LHC now]</p>
<p>Throughout the 1988-89 run, CDF was in a kind of race with &#8230; UA2 &#8230; at CERN &#8230; CDF won this &#8220;race&#8221; early in 1989, not by finding the top, but by showing &#8230; a top mass limit that ruled out its discovery by UA2 &#8230; [ similar to LHC winning the Higgs race when its mass appeared to be at beyond the reach of Fermilab]</p>
<p>around &#8230; 1991 &#8230; Kondo analyzed &#8230; the first &#8230; published &#8230; CDF dilepton event &#8230; from the 1988-89 data &#8230; Kondo found that the event could be reconstructed as the decay of a top-antitop pair, with a top mass of around 130 GeV/c^2, but &#8220;it has a very broad error&#8221; &#8230; Kondo &#8230; wanted to publish &#8230;[a]&#8230; paper in PRL &#8230; The paper met resistance from the collaboration, who felt it too closely resembled a top discovery claim &#8230; Kondo &#8220;didn&#8217;t make &#8230; trouble&#8221;, and instead published the paper in the Journal of the Physical Society of Japan &#8230;</p>
<p>In 1991 &#8230; Goldstein and Dalitz  &#8230; were trying to apply their method [of data analysis] to the first CDF dilepton event &#8230;[so they]&#8230; asked &#8230; Sliwa &#8230; for &#8230; help &#8230;</p>
<p>Goldstein and Sliwa &#8230; presented results at a heavy flavors group meeting in April [1992] &#8230; showing a bump in the probability distribution at a top-quark mass of about 120 GeV/c^2 &#8230; After that, according to Sliwa, &#8220;Goldstein was told not to come to Top Group meetings,&#8221; a decision that Sliwa believed was &#8220;highly improper&#8221; &#8230;</p>
<p>the July 24 [1992] issue of Science &#8230; described the position of Dalitz and Goldstein &#8230; &#8220;They think the patterns they found look suspiciously, though not unambiguously, like the top quark and deserve further analysis.&#8221; CDF, the article noted, &#8220;isn&#8217;t impressed&#8221; &#8230; The Science article described Dalitz and Goldstein as having &#8220;gained access to unpublished, partially analyzed CDF data only when Krys Sliwa, a member of the group, shared it without telling his colleagues.&#8221; &#8230; Goldstein denied both the sense of furtiveness and and secrecy conveyed by the Science article&#8230;</p>
<p>In June of 1992 &#8230; the run designated &#8220;Ia&#8221; began &#8230;</p>
<p>On October 29, 1992, just prior to the meeting of the &#8230; DPF &#8230; CDF recorded an event that looked strikingly like an e &#8211; mu top decay &#8230; In fact, although it was not known at the time, one of the jets in this event would be tagged by both the SVX and SLT b-tagging algorithms &#8230; some collaboration members even regarded the event by itself as worthy of publication as a top-quark event &#8230; the event, &#8230; known as &#8220;the DPF event&#8221;, would be shown at the meeting &#8230; No claim would be made what the event signified &#8230;</p>
<p>On April 26, 1994, &#8230; CDF &#8230; release[d] &#8230; a paper describing &#8220;evidence for top quark production&#8221; &#8230; D-zero did not claim to have established such evidence &#8230;&#8221;.</p>
<p>Some questions that come to mind:</p>
<p>1 &#8211; How will LHC deal with release of individual event data, to avoid controversies and yet permit outsiders to contribute their methods and interpretations,<br />
in the light of the fact that the Kondo and Dalitz/Goldstein/Sliwa methods of analysis were (and still are) useful techniques developed outside the collaboration ?</p>
<p>2 &#8211; How will LHC deal with release of its internal analyses, bearing in mind that the DPF event was released in 1992 and it was not until 1994 that a discovery &#8220;evidence&#8221; paper was released ?</p>
<p>Tony Smith<br />
<a href="http://www.valdostamuseum.org/hamsmith/" rel="nofollow">http://www.valdostamuseum.org/hamsmith/</a></p>
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