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	<title>Comments on: Bump Hunting (Redux)</title>
	<atom:link href="http://cosmicvariance.com/2007/10/22/bump-hunting-redux/feed/" rel="self" type="application/rss+xml" />
	<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/</link>
	<description>Random samplings from a universe of ideas</description>
	<pubDate>Sat, 30 Aug 2008 00:29:58 +0000</pubDate>
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		<item>
		<title>By: tommaso dorigo</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-305998</link>
		<dc:creator>tommaso dorigo</dc:creator>
		<pubDate>Sun, 09 Dec 2007 22:43:40 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-305998</guid>
		<description>Hi John,

I let a few weeks pass before pitching in on this, now that fewer eyes are looking. What I really would like to know is the details of the modeling of the QCD background, the fat red histogram that is responsible for the shape of the falling spectrum at high reconstructed mass.

Because, if I am not mistaken, the fact that you now see no excess is due to a remodeling of the QCD background (which used to be quite a bit leaner in the 1/fb analysis). So I really wonder, was it really a statistical fluctuation or a systematic underestimate of the background ?

Sorry for being quite direct... I decided not to post on this issue in my blog and just ask you here. If the new QCD model is better than the old one it is entirely to your credit, not the other way round. I think you, Anton and the others did a terrific job and I cannot see a way to improve the analysis.

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>Hi John,</p>
<p>I let a few weeks pass before pitching in on this, now that fewer eyes are looking. What I really would like to know is the details of the modeling of the QCD background, the fat red histogram that is responsible for the shape of the falling spectrum at high reconstructed mass.</p>
<p>Because, if I am not mistaken, the fact that you now see no excess is due to a remodeling of the QCD background (which used to be quite a bit leaner in the 1/fb analysis). So I really wonder, was it really a statistical fluctuation or a systematic underestimate of the background ?</p>
<p>Sorry for being quite direct&#8230; I decided not to post on this issue in my blog and just ask you here. If the new QCD model is better than the old one it is entirely to your credit, not the other way round. I think you, Anton and the others did a terrific job and I cannot see a way to improve the analysis.</p>
<p>Cheers,<br />
T.</p>
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		<title>By: Thomas D</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303314</link>
		<dc:creator>Thomas D</dc:creator>
		<pubDate>Tue, 30 Oct 2007 18:19:04 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303314</guid>
		<description>I'm not sure I like the smell of the phrase 'to catch wind of breaking news'...</description>
		<content:encoded><![CDATA[<p>I&#8217;m not sure I like the smell of the phrase &#8216;to catch wind of breaking news&#8217;&#8230;</p>
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	<item>
		<title>By: loses to monkeys</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303085</link>
		<dc:creator>loses to monkeys</dc:creator>
		<pubDate>Sat, 27 Oct 2007 18:28:32 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303085</guid>
		<description>what's plotted on the y axis of those graphs? people never label axis these days!</description>
		<content:encoded><![CDATA[<p>what&#8217;s plotted on the y axis of those graphs? people never label axis these days!</p>
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		<title>By: jlm</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303028</link>
		<dc:creator>jlm</dc:creator>
		<pubDate>Fri, 26 Oct 2007 12:27:48 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303028</guid>
		<description>Hi John,

I'm confused. If I look at the paper you linked to describing this analysis
I see that the combined efficiency listed for a 90 (250) gev higgs is 1.0% (3.1%).
And the cdf higgs webpage has a paper describing the 1.0/fb analysis which
lists the combined efficiency for the same masses as 1.1% (3.3%).  Also, the
ratio of the total number of predicted taus faking jets in the two analyses is 1.6 (slightly less than the 1.8 that comes just from luminosity scaling).

So it doesn't appear that a looser event selection has led to increased predictions for the signal or the fake background.  However, as I wrote in my previous post, it looks like the prediction for the jet faking tau background in the mass region the excess was observed in the 1.0/fb analysis has increased by 3.5 instead of 1.8.  Did I misunderstand your answer?</description>
		<content:encoded><![CDATA[<p>Hi John,</p>
<p>I&#8217;m confused. If I look at the paper you linked to describing this analysis<br />
I see that the combined efficiency listed for a 90 (250) gev higgs is 1.0% (3.1%).<br />
And the cdf higgs webpage has a paper describing the 1.0/fb analysis which<br />
lists the combined efficiency for the same masses as 1.1% (3.3%).  Also, the<br />
ratio of the total number of predicted taus faking jets in the two analyses is 1.6 (slightly less than the 1.8 that comes just from luminosity scaling).</p>
<p>So it doesn&#8217;t appear that a looser event selection has led to increased predictions for the signal or the fake background.  However, as I wrote in my previous post, it looks like the prediction for the jet faking tau background in the mass region the excess was observed in the 1.0/fb analysis has increased by 3.5 instead of 1.8.  Did I misunderstand your answer?</p>
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		<title>By: Eric</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303013</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Fri, 26 Oct 2007 03:23:12 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303013</guid>
		<description>John, you're right--after rereading your posts I agree that you were more fair than I gave you credit for.  Guess I succumbed to the usual irresistible temptation of over-sarcasm (it's quite enjoyable).  ;)</description>
		<content:encoded><![CDATA[<p>John, you&#8217;re right&#8211;after rereading your posts I agree that you were more fair than I gave you credit for.  Guess I succumbed to the usual irresistible temptation of over-sarcasm (it&#8217;s quite enjoyable).  <img src='http://cosmicvariance.com/wp-includes/images/smilies/icon_wink.gif' alt=';)' class='wp-smiley' /></p>
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		<title>By: Brian Drell</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303008</link>
		<dc:creator>Brian Drell</dc:creator>
		<pubDate>Fri, 26 Oct 2007 01:45:54 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-303008</guid>
		<description>Glad to know LHC hasn't lost usefulness before they even collide beam.

;)</description>
		<content:encoded><![CDATA[<p>Glad to know LHC hasn&#8217;t lost usefulness before they even collide beam.</p>
<p> <img src='http://cosmicvariance.com/wp-includes/images/smilies/icon_wink.gif' alt=';)' class='wp-smiley' /></p>
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		<title>By: John</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302994</link>
		<dc:creator>John</dc:creator>
		<pubDate>Thu, 25 Oct 2007 17:35:57 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302994</guid>
		<description>Hi jlm (#22): the reason the background did not scale is that we loosened our selection a bit to get better sensitivity (more backgorund but more signal too...)

Eric, #25, apaprently you didn't read my original posts.  I think if you go back and do your homework, you can tone down the sarcasm a bit.   I never hyped anything...the media did.  It was a typical cycle with this sort of fluctuation.  The main point is if the Higgs *had* been there this is *exactly* how it would have appeared.  My first post, and this one, was all about how important it is to remain skeptical, while being human.  This is exciting!  Are you saying you never expect to see a Higgs anywhere?

In response to your comment #28, our estimate of the probability of a fluctuation *of course* took into account that a fluctuation could have been anwhere.  This was discussed in the first posts, which, as I say, you really should take the tme to read.  I stand by every word I wrote.</description>
		<content:encoded><![CDATA[<p>Hi jlm (#22): the reason the background did not scale is that we loosened our selection a bit to get better sensitivity (more backgorund but more signal too&#8230;)</p>
<p>Eric, #25, apaprently you didn&#8217;t read my original posts.  I think if you go back and do your homework, you can tone down the sarcasm a bit.   I never hyped anything&#8230;the media did.  It was a typical cycle with this sort of fluctuation.  The main point is if the Higgs *had* been there this is *exactly* how it would have appeared.  My first post, and this one, was all about how important it is to remain skeptical, while being human.  This is exciting!  Are you saying you never expect to see a Higgs anywhere?</p>
<p>In response to your comment #28, our estimate of the probability of a fluctuation *of course* took into account that a fluctuation could have been anwhere.  This was discussed in the first posts, which, as I say, you really should take the tme to read.  I stand by every word I wrote.</p>
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		<title>By: Eric</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302959</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Thu, 25 Oct 2007 02:01:04 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302959</guid>
		<description>Furthermore, there is an experimental bias because one selectively pays attention to fluctuations that occur in quantities of interest and ignores fluctuations elsewhere.  An experimenter should really consider the probability of getting a 2-sigma fluctuation *anywhere* (not just here), which is pretty high due to combinatorics.  J. Conway is reputed to be a statistics guru, so maybe that was done, I'm not sure.</description>
		<content:encoded><![CDATA[<p>Furthermore, there is an experimental bias because one selectively pays attention to fluctuations that occur in quantities of interest and ignores fluctuations elsewhere.  An experimenter should really consider the probability of getting a 2-sigma fluctuation *anywhere* (not just here), which is pretty high due to combinatorics.  J. Conway is reputed to be a statistics guru, so maybe that was done, I&#8217;m not sure.</p>
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		<title>By: Eric</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302957</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Thu, 25 Oct 2007 01:48:37 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302957</guid>
		<description>Neil, there's no obvious way to know, assuming all other checks have been made.  

A 3-sigma effect is decent, but any good particle experimentalist will tell you that 5 sigma is the gold standard.  Many people (especially theorists) ask:  a 3-sigma fluctuation is so statistically unlikely already--why need 5?  The answer:  Well, the probability of a 5 sigma is exponentially suppressed compared to 3 sigma.  But more saliently, it also offers robustness against mistakes in error estimation.  For example, if you accidentally underestimate your error by a factor of 2, your great 3-sigma effect now becomes a 1.5 sigma effect, which happens quite frequently.  Similar reasoning applies to error estimation from Monte Carlo, which may not properly model new physics, etc.

The point of having 5 sigma is so that claims of discovery are robust against not only statistical fluctuations, but also against experimenter-related mistakes.  Until one is near that, I think it's misleading to imply a near-discovery (as it seemed to me was done here at CV, New Scientist, etc.)  There was no legitimate reason to hype up the result so much.</description>
		<content:encoded><![CDATA[<p>Neil, there&#8217;s no obvious way to know, assuming all other checks have been made.  </p>
<p>A 3-sigma effect is decent, but any good particle experimentalist will tell you that 5 sigma is the gold standard.  Many people (especially theorists) ask:  a 3-sigma fluctuation is so statistically unlikely already&#8211;why need 5?  The answer:  Well, the probability of a 5 sigma is exponentially suppressed compared to 3 sigma.  But more saliently, it also offers robustness against mistakes in error estimation.  For example, if you accidentally underestimate your error by a factor of 2, your great 3-sigma effect now becomes a 1.5 sigma effect, which happens quite frequently.  Similar reasoning applies to error estimation from Monte Carlo, which may not properly model new physics, etc.</p>
<p>The point of having 5 sigma is so that claims of discovery are robust against not only statistical fluctuations, but also against experimenter-related mistakes.  Until one is near that, I think it&#8217;s misleading to imply a near-discovery (as it seemed to me was done here at CV, New Scientist, etc.)  There was no legitimate reason to hype up the result so much.</p>
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		<title>By: Neil B.</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302955</link>
		<dc:creator>Neil B.</dc:creator>
		<pubDate>Thu, 25 Oct 2007 01:04:00 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302955</guid>
		<description>OK... Eric (or anyone) have we advanced in our ability to figure whether a given marginal signal is likely real or just noise etc?  The basic simple math has been known and likely not changed for awhile, but I figure there have been advances (whether in the math or the computational power.)  I don't hear much about it.</description>
		<content:encoded><![CDATA[<p>OK&#8230; Eric (or anyone) have we advanced in our ability to figure whether a given marginal signal is likely real or just noise etc?  The basic simple math has been known and likely not changed for awhile, but I figure there have been advances (whether in the math or the computational power.)  I don&#8217;t hear much about it.</p>
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		<title>By: Eric</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302950</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Thu, 25 Oct 2007 00:20:56 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302950</guid>
		<description>The bump vanished.  Surprise!...NOT.

This is why experimentalists overeager for acclaim shouldn't hype up their small and insignificant fluctuations in the public domain, especially to the general public (that includes theorists), lest the unsuspecting public (again that includes theorists) should get unreasonably excited.  Any experimentalist with half an once of skepticism would know that 2 sigma fluctuations are just that and shouldn't be publicized as an impending discovery.

Well, at least I get to say "I told you so" to all my friends.</description>
		<content:encoded><![CDATA[<p>The bump vanished.  Surprise!&#8230;NOT.</p>
<p>This is why experimentalists overeager for acclaim shouldn&#8217;t hype up their small and insignificant fluctuations in the public domain, especially to the general public (that includes theorists), lest the unsuspecting public (again that includes theorists) should get unreasonably excited.  Any experimentalist with half an once of skepticism would know that 2 sigma fluctuations are just that and shouldn&#8217;t be publicized as an impending discovery.</p>
<p>Well, at least I get to say &#8220;I told you so&#8221; to all my friends.</p>
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		<title>By: Nonnormalizable</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302942</link>
		<dc:creator>Nonnormalizable</dc:creator>
		<pubDate>Wed, 24 Oct 2007 22:29:25 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302942</guid>
		<description>Hey Neil B., this thread doesn't seem like the best venue for your question, but anyway: I think (in nonrelativistic QM anyway) that such a process as you describe, with a detector that has probability P of each detection being true, could easily be analyzed as collapsing the wave function from Psi to an incoherent mixture of (1-P)*Psi + P*delta function. I'm not aware of such a thing giving anything interesting, but I'm not an expert.</description>
		<content:encoded><![CDATA[<p>Hey Neil B., this thread doesn&#8217;t seem like the best venue for your question, but anyway: I think (in nonrelativistic QM anyway) that such a process as you describe, with a detector that has probability P of each detection being true, could easily be analyzed as collapsing the wave function from Psi to an incoherent mixture of (1-P)*Psi + P*delta function. I&#8217;m not aware of such a thing giving anything interesting, but I&#8217;m not an expert.</p>
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		<title>By: Hiranya</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302924</link>
		<dc:creator>Hiranya</dc:creator>
		<pubDate>Wed, 24 Oct 2007 11:20:41 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302924</guid>
		<description>I have really enjoyed this series of posts! Please keep it coming :)</description>
		<content:encoded><![CDATA[<p>I have really enjoyed this series of posts! Please keep it coming <img src='http://cosmicvariance.com/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /></p>
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		<title>By: jlm</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302921</link>
		<dc:creator>jlm</dc:creator>
		<pubDate>Wed, 24 Oct 2007 10:29:12 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302921</guid>
		<description>Hi John,

Thanks for the update.  If I read the prediction for jets faking
a tau in the region 120-150 gev it looks like it went from about
10 in the 1/fb analysis to ~35 in the 1.8/fb analysis.  What is
the reason this prediction didn't scale?</description>
		<content:encoded><![CDATA[<p>Hi John,</p>
<p>Thanks for the update.  If I read the prediction for jets faking<br />
a tau in the region 120-150 gev it looks like it went from about<br />
10 in the 1/fb analysis to ~35 in the 1.8/fb analysis.  What is<br />
the reason this prediction didn&#8217;t scale?</p>
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	<item>
		<title>By: Jason Dick</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302910</link>
		<dc:creator>Jason Dick</dc:creator>
		<pubDate>Wed, 24 Oct 2007 05:50:17 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302910</guid>
		<description>P.S.
The problem in post #20 I was alluding to was in response to post #19.  the rest of the post was in response to post #18.</description>
		<content:encoded><![CDATA[<p>P.S.<br />
The problem in post #20 I was alluding to was in response to post #19.  the rest of the post was in response to post #18.</p>
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		<title>By: Jason Dick</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302907</link>
		<dc:creator>Jason Dick</dc:creator>
		<pubDate>Wed, 24 Oct 2007 05:34:01 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302907</guid>
		<description>Well, I'm really not sure what you mean.  I'm into cosmology, and basically only have the one graduate course series in field theory to draw on here, so I'll just leave it at saying that I don't even understand the problem you are alluding to.

As for renormalization, though, from what I remember of renormalization, it really isn't a problem with respect to energies blowing up location-wise.  It has to do with certain components in Feynman diagrams giving infinite results that come from taking the integrals to infinite energy (loop diagrams, specifically).  This is solved by suggesting that there is some physics beyond a certain energy that we just don't understand, so we should cut off our integrals, use a dummy parameter to represent the value of the integral out to infinity, and use experiment to fix the value of this dummy parameter.  Then, as long as we can show that our prescription of renormalization is independent of the cutoff energy we choose, this should be a valid thing to do.  All that remains after this is to measure whatever parameters are required in renormalization theory using one set of experiments, and see if the corroborate with the same parameters measured in a different experiment using different interactions.

And no, I don't think it has anything to do with them not being able to have energy.  I'm honestly not clear on what the theoretical problems with giving particles mass are.  But I do know that they would, in terms of energy/momentum, act exactly like photons at a "fundamental" level, before adding interactions to the theory.  It could, of course, simply be that we just don't understand the nature of mass, which is why it'd be at least as interesting to find no Higgs as it would be to find one.</description>
		<content:encoded><![CDATA[<p>Well, I&#8217;m really not sure what you mean.  I&#8217;m into cosmology, and basically only have the one graduate course series in field theory to draw on here, so I&#8217;ll just leave it at saying that I don&#8217;t even understand the problem you are alluding to.</p>
<p>As for renormalization, though, from what I remember of renormalization, it really isn&#8217;t a problem with respect to energies blowing up location-wise.  It has to do with certain components in Feynman diagrams giving infinite results that come from taking the integrals to infinite energy (loop diagrams, specifically).  This is solved by suggesting that there is some physics beyond a certain energy that we just don&#8217;t understand, so we should cut off our integrals, use a dummy parameter to represent the value of the integral out to infinity, and use experiment to fix the value of this dummy parameter.  Then, as long as we can show that our prescription of renormalization is independent of the cutoff energy we choose, this should be a valid thing to do.  All that remains after this is to measure whatever parameters are required in renormalization theory using one set of experiments, and see if the corroborate with the same parameters measured in a different experiment using different interactions.</p>
<p>And no, I don&#8217;t think it has anything to do with them not being able to have energy.  I&#8217;m honestly not clear on what the theoretical problems with giving particles mass are.  But I do know that they would, in terms of energy/momentum, act exactly like photons at a &#8220;fundamental&#8221; level, before adding interactions to the theory.  It could, of course, simply be that we just don&#8217;t understand the nature of mass, which is why it&#8217;d be at least as interesting to find no Higgs as it would be to find one.</p>
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		<title>By: Neil B.</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302895</link>
		<dc:creator>Neil B.</dc:creator>
		<pubDate>Wed, 24 Oct 2007 02:33:43 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302895</guid>
		<description>Jason, if you aren't feeling too condescended to in my "God" post, (sorry), I still am looking for a good answer to my question about effect of unreliable detectors on wave functions in general.  John took it too much direct to his experiments, and I want to know the general implications, tx.</description>
		<content:encoded><![CDATA[<p>Jason, if you aren&#8217;t feeling too condescended to in my &#8220;God&#8221; post, (sorry), I still am looking for a good answer to my question about effect of unreliable detectors on wave functions in general.  John took it too much direct to his experiments, and I want to know the general implications, tx.</p>
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		<title>By: Neil B.</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302875</link>
		<dc:creator>Neil B.</dc:creator>
		<pubDate>Tue, 23 Oct 2007 22:06:18 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302875</guid>
		<description>John, Jason, thanks.  Now, what I think is really ironic: that you say, 
"if we attempt to add mass directly to particles, field theory doesn’t work, ... then all particles must, on a fundamental level, have zero mass,..."  OK, but then the problem that required "renormalization" was apparently just the opposite: the field/interaction energies around a particle (at least, a charged one like an electron) were infinite (and energy is equivalent to mass), which is just weird.  BTW, I assume you all mean Higgs must be needed to give "rest mass", for otherwise the Higgs-free "massless" particles wouldn't even have energy (the way photons do) - ?</description>
		<content:encoded><![CDATA[<p>John, Jason, thanks.  Now, what I think is really ironic: that you say,<br />
&#8220;if we attempt to add mass directly to particles, field theory doesn’t work, &#8230; then all particles must, on a fundamental level, have zero mass,&#8230;&#8221;  OK, but then the problem that required &#8220;renormalization&#8221; was apparently just the opposite: the field/interaction energies around a particle (at least, a charged one like an electron) were infinite (and energy is equivalent to mass), which is just weird.  BTW, I assume you all mean Higgs must be needed to give &#8220;rest mass&#8221;, for otherwise the Higgs-free &#8220;massless&#8221; particles wouldn&#8217;t even have energy (the way photons do) - ?</p>
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		<title>By: John</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302872</link>
		<dc:creator>John</dc:creator>
		<pubDate>Tue, 23 Oct 2007 21:19:57 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302872</guid>
		<description>Again, Neil, the types of quantum-level fluctuations in the detector which you are talking about don't really affect us, at least not in the process of detecting these high-energy particles.  It is certainly true that quantum mechanics reigns supreme in the "initial state" or "hard collision process" that we are looking for.   And we do quite detailed calculations of those effects, which can include the spin polarization states of the outgoing particles.  But once the particles leave the interaction region, and leave their signatures in our detector, we really don't need to account for quantum correlations between them in terms of the detector efficiency.  The photons hitting our lead-based calorimeter have 20 billion times more energy than visible light photons...no wave-diffraction or quantum-uncertainty effects here!   They hit the lead nuclei and basically shatter into a huge number of pieces (an "electromagnetic shower").  Our uncertainty on their position and momentum is many orders of magnitude away from the quantum measurement limit.

All this having been said there have been some collider tests of Bell's Inequality proposed using the final state polarization correlations of the outgoing particles.  But these effects play no role in detecting (or not) high energy hadrons, electrons, muons, photons, etc.   Our inefficiencies are more of the nature that the electronics was not working properly...</description>
		<content:encoded><![CDATA[<p>Again, Neil, the types of quantum-level fluctuations in the detector which you are talking about don&#8217;t really affect us, at least not in the process of detecting these high-energy particles.  It is certainly true that quantum mechanics reigns supreme in the &#8220;initial state&#8221; or &#8220;hard collision process&#8221; that we are looking for.   And we do quite detailed calculations of those effects, which can include the spin polarization states of the outgoing particles.  But once the particles leave the interaction region, and leave their signatures in our detector, we really don&#8217;t need to account for quantum correlations between them in terms of the detector efficiency.  The photons hitting our lead-based calorimeter have 20 billion times more energy than visible light photons&#8230;no wave-diffraction or quantum-uncertainty effects here!   They hit the lead nuclei and basically shatter into a huge number of pieces (an &#8220;electromagnetic shower&#8221;).  Our uncertainty on their position and momentum is many orders of magnitude away from the quantum measurement limit.</p>
<p>All this having been said there have been some collider tests of Bell&#8217;s Inequality proposed using the final state polarization correlations of the outgoing particles.  But these effects play no role in detecting (or not) high energy hadrons, electrons, muons, photons, etc.   Our inefficiencies are more of the nature that the electronics was not working properly&#8230;</p>
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		<title>By: Jason Dick</title>
		<link>http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302871</link>
		<dc:creator>Jason Dick</dc:creator>
		<pubDate>Tue, 23 Oct 2007 21:18:49 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/2007/10/22/bump-hunting-redux/#comment-302871</guid>
		<description>Neil B.,

The short answer is that if we attempt to add mass directly to particles, field theory doesn't work, and least in the standard model formalism.  So, if field theory as we understand it is correct, then all particles must, on a fundamental level, have zero mass, and there must be some physical mechanism that gives them apparent mass.</description>
		<content:encoded><![CDATA[<p>Neil B.,</p>
<p>The short answer is that if we attempt to add mass directly to particles, field theory doesn&#8217;t work, and least in the standard model formalism.  So, if field theory as we understand it is correct, then all particles must, on a fundamental level, have zero mass, and there must be some physical mechanism that gives them apparent mass.</p>
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