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	<title>Comments on: Most Surprising LHC Discovery?</title>
	<atom:link href="http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/feed/" rel="self" type="application/rss+xml" />
	<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/</link>
	<description>Random samplings from a universe of ideas</description>
	<pubDate>Thu, 16 Oct 2008 03:12:05 +0000</pubDate>
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		<title>By: B</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-110663</link>
		<dc:creator>B</dc:creator>
		<pubDate>Fri, 04 Aug 2006 23:36:43 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-110663</guid>
		<description>Hi JoAnne,

Thanks, I see. Was thinking too complicatd :-) Have a nice weekend, B.</description>
		<content:encoded><![CDATA[<p>Hi JoAnne,</p>
<p>Thanks, I see. Was thinking too complicatd <img src='http://cosmicvariance.com/wp-includes/images/smilies/icon_smile.gif' alt=':-)' class='wp-smiley' /> Have a nice weekend, B.</p>
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		<title>By: Count Iblis</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-110276</link>
		<dc:creator>Count Iblis</dc:creator>
		<pubDate>Thu, 03 Aug 2006 15:33:02 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-110276</guid>
		<description>Also interesting:

&lt;a href="http://arxiv.org/abs/hep-ph/0005238" rel="nofollow"&gt;Discovering mirror particles at the Large Hadron Collider and the implied cold universe&lt;/a&gt;

&lt;blockquote&gt;The Mirror Matter or Exact Parity Model sees every standard particle, including the physical neutral Higgs boson, paired with a parity partner. The unbroken parity symmetry forces the mass eigenstate Higgs bosons to be maximal mixtures of the ordinary and mirror Higgs bosons. Each of these mass eigenstates will therefore decay 50% of the time into invisible mirror particles, providing a clear and interesting signature for the Large Hadron Collider (LHC) which could thus establish the existence of the mirror world. However, for this effect to be observable the mass difference between the two eigenstates must be sufficiently large. In this paper, we study cosmological constraints from Big Bang Nucleosynthesis on the mass difference parameter. We find that the temperature of the radiation dominated (RD) phase of the universe should never have exceeded a few 10's of GeV if the mass difference is to be observable at the LHC. Chaotic inflation with very inefficient reheating provides an example of how such a cosmology could arise. We conclude that the LHC could thus discover the mirror world and simultaneously establish an upper bound on the temperature of the RD phase of the universe. &lt;/blockquote&gt;</description>
		<content:encoded><![CDATA[<p>Also interesting:</p>
<p><a href="http://arxiv.org/abs/hep-ph/0005238" rel="nofollow">Discovering mirror particles at the Large Hadron Collider and the implied cold universe</a></p>
<blockquote><p>The Mirror Matter or Exact Parity Model sees every standard particle, including the physical neutral Higgs boson, paired with a parity partner. The unbroken parity symmetry forces the mass eigenstate Higgs bosons to be maximal mixtures of the ordinary and mirror Higgs bosons. Each of these mass eigenstates will therefore decay 50% of the time into invisible mirror particles, providing a clear and interesting signature for the Large Hadron Collider (LHC) which could thus establish the existence of the mirror world. However, for this effect to be observable the mass difference between the two eigenstates must be sufficiently large. In this paper, we study cosmological constraints from Big Bang Nucleosynthesis on the mass difference parameter. We find that the temperature of the radiation dominated (RD) phase of the universe should never have exceeded a few 10&#8217;s of GeV if the mass difference is to be observable at the LHC. Chaotic inflation with very inefficient reheating provides an example of how such a cosmology could arise. We conclude that the LHC could thus discover the mirror world and simultaneously establish an upper bound on the temperature of the RD phase of the universe. </p></blockquote>
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		<title>By: JoAnne</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-110171</link>
		<dc:creator>JoAnne</dc:creator>
		<pubDate>Wed, 02 Aug 2006 23:26:14 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-110171</guid>
		<description>Hi B:

The masses of the KK graviton excitations in the Randall-Sundrum model are proportional to the roots of the J_1 Bessel function.  The first root, which sets the scale for the first excitation, has a value of 3.83.  One of the main signatures for a warped extra dimension is that the KK states are not evenly spaced, but have spacings proportional to roots of Bessel functions. As I said, 'Graviton383' clearly knows his/her Randall-Sundrum phenomenology.</description>
		<content:encoded><![CDATA[<p>Hi B:</p>
<p>The masses of the KK graviton excitations in the Randall-Sundrum model are proportional to the roots of the J_1 Bessel function.  The first root, which sets the scale for the first excitation, has a value of 3.83.  One of the main signatures for a warped extra dimension is that the KK states are not evenly spaced, but have spacings proportional to roots of Bessel functions. As I said, &#8216;Graviton383&#8242; clearly knows his/her Randall-Sundrum phenomenology.</p>
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		<title>By: B</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-110167</link>
		<dc:creator>B</dc:creator>
		<pubDate>Wed, 02 Aug 2006 22:52:07 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-110167</guid>
		<description>Hi "graviton",

well, I was about to give you the reference, but I guess you are familiar with it ;-)

&lt;i&gt;I donâ€™t necessarity believe that microscopic BH physics is T invariantâ€¦ Even macroscopic BH physics is not T invariant since Hawking radiation is a statistical process but stellar collapse is not.&lt;/i&gt;

Yep, that's the same answer I give when someone comes up with that point. That's what my brain says. However, my stomach expects the universe to be nice and pretty, such that it allows elementary process back as well as forth. So, I agree with you that relics aren't excluded, but to be honest, I just don't believe in it.

Best, B.

PS 
JoAnne: &lt;i&gt;the fact that the very name graviton383 shows intimate and deep knowledge of the phenomenology of the Randall-Sundrum model&lt;/i&gt; 
I don't get it, can you give me a hint?</description>
		<content:encoded><![CDATA[<p>Hi &#8220;graviton&#8221;,</p>
<p>well, I was about to give you the reference, but I guess you are familiar with it <img src='http://cosmicvariance.com/wp-includes/images/smilies/icon_wink.gif' alt=';-)' class='wp-smiley' /> </p>
<p><i>I donâ€™t necessarity believe that microscopic BH physics is T invariantâ€¦ Even macroscopic BH physics is not T invariant since Hawking radiation is a statistical process but stellar collapse is not.</i></p>
<p>Yep, that&#8217;s the same answer I give when someone comes up with that point. That&#8217;s what my brain says. However, my stomach expects the universe to be nice and pretty, such that it allows elementary process back as well as forth. So, I agree with you that relics aren&#8217;t excluded, but to be honest, I just don&#8217;t believe in it.</p>
<p>Best, B.</p>
<p>PS<br />
JoAnne: <i>the fact that the very name graviton383 shows intimate and deep knowledge of the phenomenology of the Randall-Sundrum model</i><br />
I don&#8217;t get it, can you give me a hint?</p>
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		<title>By: Haelfix</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-110099</link>
		<dc:creator>Haelfix</dc:creator>
		<pubDate>Wed, 02 Aug 2006 12:42:42 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-110099</guid>
		<description>How about this one.. The existence of a myriad set of completely random scalars not covered by any existing model and with no apparent symmetry principle that governs them.

That would be extraordinarily bad for a number of reasons.

But yea the nondiscovery of the Higgs or alternatives (and im skeptical about some of those proposals) would be catastrophic.  If for no other reason than they are more or less guarenteed to be there by no lose theorems.  The electroweak sector would then be formally inconsistent and we would be stuck.</description>
		<content:encoded><![CDATA[<p>How about this one.. The existence of a myriad set of completely random scalars not covered by any existing model and with no apparent symmetry principle that governs them.</p>
<p>That would be extraordinarily bad for a number of reasons.</p>
<p>But yea the nondiscovery of the Higgs or alternatives (and im skeptical about some of those proposals) would be catastrophic.  If for no other reason than they are more or less guarenteed to be there by no lose theorems.  The electroweak sector would then be formally inconsistent and we would be stuck.</p>
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		<title>By: graviton383</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-110004</link>
		<dc:creator>graviton383</dc:creator>
		<pubDate>Wed, 02 Aug 2006 09:22:18 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-110004</guid>
		<description>Mark: thanks for your fierce loyalty!</description>
		<content:encoded><![CDATA[<p>Mark: thanks for your fierce loyalty!</p>
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		<title>By: JoAnne</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109936</link>
		<dc:creator>JoAnne</dc:creator>
		<pubDate>Wed, 02 Aug 2006 04:12:56 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109936</guid>
		<description>Indeed, I am still gonna believe that graviton383 is anonymous.....except for the fact that the very name graviton383 shows intimate and deep knowledge of the phenomenology of the Randall-Sundrum model.

Hack, comment #1:  The real problem is that almost nobody is expecting the unexpected.  The majority think that not only will SUSY show up, but it will be our most studied benchmark point SUSY SPS1a!   If SUSY shows up  and it's not the benchmark point in parameter space we have studied well (i.e., point SPS1a) we might be terribly confused.</description>
		<content:encoded><![CDATA[<p>Indeed, I am still gonna believe that graviton383 is anonymous&#8230;..except for the fact that the very name graviton383 shows intimate and deep knowledge of the phenomenology of the Randall-Sundrum model.</p>
<p>Hack, comment #1:  The real problem is that almost nobody is expecting the unexpected.  The majority think that not only will SUSY show up, but it will be our most studied benchmark point SUSY SPS1a!   If SUSY shows up  and it&#8217;s not the benchmark point in parameter space we have studied well (i.e., point SPS1a) we might be terribly confused.</p>
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		<title>By: Mark</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109931</link>
		<dc:creator>Mark</dc:creator>
		<pubDate>Wed, 02 Aug 2006 03:26:48 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109931</guid>
		<description>Can't believe you gave yourself away Tom! We get to see the email address, but I would never have given you up, never I tell you!</description>
		<content:encoded><![CDATA[<p>Can&#8217;t believe you gave yourself away Tom! We get to see the email address, but I would never have given you up, never I tell you!</p>
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		<title>By: graviton383</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109930</link>
		<dc:creator>graviton383</dc:creator>
		<pubDate>Wed, 02 Aug 2006 03:05:02 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109930</guid>
		<description>Hi B:

Thanks for you comments, I have heard these arguments 
but I don't necessarity believe that microscopic BH physics is T invariant... Even macroscopic BH physics is not T invariant since Hawking radiation is a statistical process but stellar collapse is not. Thanks for the 
reference to the work of Rizzo..I am very familiar with it..I wrote it.</description>
		<content:encoded><![CDATA[<p>Hi B:</p>
<p>Thanks for you comments, I have heard these arguments<br />
but I don&#8217;t necessarity believe that microscopic BH physics is T invariant&#8230; Even macroscopic BH physics is not T invariant since Hawking radiation is a statistical process but stellar collapse is not. Thanks for the<br />
reference to the work of Rizzo..I am very familiar with it..I wrote it.</p>
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		<title>By: B</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109926</link>
		<dc:creator>B</dc:creator>
		<pubDate>Wed, 02 Aug 2006 02:06:17 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109926</guid>
		<description>Hi graviton,

&lt;i&gt;I see no reason based on existing data why such things canâ€™t exist since we donâ€™t know the threshold mass scale or the number of extra dimensions&lt;/i&gt;

Yep I agree, there is a lot we don't know, and we certainly don't know for sure whether black hole relics can exist or not. Imo we know even much less about black hole evaporation than is commonly &lt;b&gt;believed&lt;/b&gt; to be "true". However, the question relics or not has not a priory anything to do with the threshold or the # of extra dims (unless you think of higher curvature corrections to GR, see e.g. work by Rizzo, there the # of extra dims is crucial). 

The  most common arguments against relics (both of which I think don't hold) are the necessity for an arbitrarily large information content (based on a misinterpretation of the black hole's entropy) and an enormous phase space for the pair production (which follows from the first argument, and therefore is also a misconception).

The reason why I don't like black hole relics is that their existence breaks time-reversal symmetry. If a black hole can be formed in a collision of two particles, I expect it should be able to decay in the reverse process.

Hi Tony,

right. But that is not the patent Horst holds. He does not want to &lt;i&gt;extract&lt;/i&gt; energy from the hole. He just wants to use it to &lt;i&gt;convert&lt;/i&gt; energy. Like a very efficient fire place, with the extra virtue that it absolutely does not care what you throw in.

Best,

B.</description>
		<content:encoded><![CDATA[<p>Hi graviton,</p>
<p><i>I see no reason based on existing data why such things canâ€™t exist since we donâ€™t know the threshold mass scale or the number of extra dimensions</i></p>
<p>Yep I agree, there is a lot we don&#8217;t know, and we certainly don&#8217;t know for sure whether black hole relics can exist or not. Imo we know even much less about black hole evaporation than is commonly <b>believed</b> to be &#8220;true&#8221;. However, the question relics or not has not a priory anything to do with the threshold or the # of extra dims (unless you think of higher curvature corrections to GR, see e.g. work by Rizzo, there the # of extra dims is crucial). </p>
<p>The  most common arguments against relics (both of which I think don&#8217;t hold) are the necessity for an arbitrarily large information content (based on a misinterpretation of the black hole&#8217;s entropy) and an enormous phase space for the pair production (which follows from the first argument, and therefore is also a misconception).</p>
<p>The reason why I don&#8217;t like black hole relics is that their existence breaks time-reversal symmetry. If a black hole can be formed in a collision of two particles, I expect it should be able to decay in the reverse process.</p>
<p>Hi Tony,</p>
<p>right. But that is not the patent Horst holds. He does not want to <i>extract</i> energy from the hole. He just wants to use it to <i>convert</i> energy. Like a very efficient fire place, with the extra virtue that it absolutely does not care what you throw in.</p>
<p>Best,</p>
<p>B.</p>
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		<title>By: Tony Smith</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109292</link>
		<dc:creator>Tony Smith</dc:creator>
		<pubDate>Tue, 01 Aug 2006 00:41:32 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109292</guid>
		<description>B said "...The more sophisticated version of the ... Horst ... patent is to throw the nuclear waste into the black hole and convert it into â€˜cleanâ€™ energy. ...". 

For prior art, see Misner, Thorne and Wheeler's book Gravitation (Freeman 1973) at page 908, Figure 33.2, 
whose caption says in part: 
"... At the dump the garbage is ... dropped toward the center of the black hole. ... As the garbage flies down the hole ... the shuttle vehicle recoils from the ejection and goes flying back out with more energy ... than it took down. ...". 

However, given the horrible mess that is USA "intellectual property" law, Horst may get his patent . 

Tony Smith
http://www.valdostamuseum.org/hamsmith/</description>
		<content:encoded><![CDATA[<p>B said &#8220;&#8230;The more sophisticated version of the &#8230; Horst &#8230; patent is to throw the nuclear waste into the black hole and convert it into â€˜cleanâ€™ energy. &#8230;&#8221;. </p>
<p>For prior art, see Misner, Thorne and Wheeler&#8217;s book Gravitation (Freeman 1973) at page 908, Figure 33.2,<br />
whose caption says in part:<br />
&#8220;&#8230; At the dump the garbage is &#8230; dropped toward the center of the black hole. &#8230; As the garbage flies down the hole &#8230; the shuttle vehicle recoils from the ejection and goes flying back out with more energy &#8230; than it took down. &#8230;&#8221;. </p>
<p>However, given the horrible mess that is USA &#8220;intellectual property&#8221; law, Horst may get his patent . </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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		<title>By: Count Iblis</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109228</link>
		<dc:creator>Count Iblis</dc:creator>
		<pubDate>Mon, 31 Jul 2006 22:51:03 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109228</guid>
		<description>Some time ago, Hawking predicted that the Higgs will be unobservable due to the effects of virtual black holes, &lt;a href="http://arxiv.org/abs/hep-th/9510029" rel="nofollow"&gt;see here.&lt;/a&gt;

&lt;blockquote&gt;One would expect spacetime to have a foam-like structure on the Planck scale with a very high topology. If spacetime is simply connected (which is assumed in this paper), the non-trivial homology occurs in dimension two, and spacetime can be regarded as being essentially the topological sum of $S^2\times S^2$ and $K3$ bubbles. Comparison with the instantons for pair creation of black holes shows that the $S^2\times S^2$ bubbles can be interpreted as closed loops of virtual black holes. It is shown that scattering in such topological fluctuations leads to loss of quantum coherence, or in other words, to a superscattering matrix $\$ $ that does not factorise into an $S$ matrix and its adjoint. This loss of quantum coherence is very small at low energies for everything except scalar fields, leading to the prediction that we may never observe the Higgs particle. Another possible observational consequence may be that the $\theta $ angle of QCD is zero without having to invoke the problematical existence of a light axion. The picture of virtual black holes given here also suggests that macroscopic black holes will evaporate down to the Planck size and then disappear in the sea of virtual black holes. 
&lt;/blockquote&gt;</description>
		<content:encoded><![CDATA[<p>Some time ago, Hawking predicted that the Higgs will be unobservable due to the effects of virtual black holes, <a href="http://arxiv.org/abs/hep-th/9510029" rel="nofollow">see here.</a></p>
<blockquote><p>One would expect spacetime to have a foam-like structure on the Planck scale with a very high topology. If spacetime is simply connected (which is assumed in this paper), the non-trivial homology occurs in dimension two, and spacetime can be regarded as being essentially the topological sum of $S^2\times S^2$ and $K3$ bubbles. Comparison with the instantons for pair creation of black holes shows that the $S^2\times S^2$ bubbles can be interpreted as closed loops of virtual black holes. It is shown that scattering in such topological fluctuations leads to loss of quantum coherence, or in other words, to a superscattering matrix $\$ $ that does not factorise into an $S$ matrix and its adjoint. This loss of quantum coherence is very small at low energies for everything except scalar fields, leading to the prediction that we may never observe the Higgs particle. Another possible observational consequence may be that the $\theta $ angle of QCD is zero without having to invoke the problematical existence of a light axion. The picture of virtual black holes given here also suggests that macroscopic black holes will evaporate down to the Planck size and then disappear in the sea of virtual black holes.
</p></blockquote>
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		<title>By: graviton383</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109022</link>
		<dc:creator>graviton383</dc:creator>
		<pubDate>Mon, 31 Jul 2006 18:19:29 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109022</guid>
		<description>B: I see no reason based on existing data why such things can't exist since we don't know the threshold mass scale or the number of extra dimensions.....</description>
		<content:encoded><![CDATA[<p>B: I see no reason based on existing data why such things can&#8217;t exist since we don&#8217;t know the threshold mass scale or the number of extra dimensions&#8230;..</p>
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		<title>By: B</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-109008</link>
		<dc:creator>B</dc:creator>
		<pubDate>Mon, 31 Jul 2006 17:45:42 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-109008</guid>
		<description>&lt;i&gt;Tony said: Why would anybody write â€œnasty commentsâ€ about hep-ph/0507138 by Bee et al ?&lt;/i&gt;

coz there are one thousand reasons why black hole relics shouldn't exist, and people kept throwing at my head how stupid I am (they still do). Most didn't get that the point of the paper wasn't to prove relics exist. I just said: if they do (and to be honest, we don't know, do we?) then what would the signature look like.


I doubt Horst took the patent out of the movie, but that was also my association... The more sophisticated version of the patent is to throw the nuclear waste into the black hole and convert it into 'clean' energy.</description>
		<content:encoded><![CDATA[<p><i>Tony said: Why would anybody write â€œnasty commentsâ€ about hep-ph/0507138 by Bee et al ?</i></p>
<p>coz there are one thousand reasons why black hole relics shouldn&#8217;t exist, and people kept throwing at my head how stupid I am (they still do). Most didn&#8217;t get that the point of the paper wasn&#8217;t to prove relics exist. I just said: if they do (and to be honest, we don&#8217;t know, do we?) then what would the signature look like.</p>
<p>I doubt Horst took the patent out of the movie, but that was also my association&#8230; The more sophisticated version of the patent is to throw the nuclear waste into the black hole and convert it into &#8216;clean&#8217; energy.</p>
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		<title>By: Qubit</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-107933</link>
		<dc:creator>Qubit</dc:creator>
		<pubDate>Sun, 30 Jul 2006 20:46:24 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-107933</guid>
		<description>Most Surprising LHC Discovery?  I would say that; a new particle will be discovered, one that has so much mass, it leave a track through the muon chambers. It will indicate, by the track it will leave, that the particle has more energy, than the experiment should have produced. The particle will also, not come from the direct result of the collision, but will be a left over remnant of something that cannot collide using just a one loop collider. 

Qubit</description>
		<content:encoded><![CDATA[<p>Most Surprising LHC Discovery?  I would say that; a new particle will be discovered, one that has so much mass, it leave a track through the muon chambers. It will indicate, by the track it will leave, that the particle has more energy, than the experiment should have produced. The particle will also, not come from the direct result of the collision, but will be a left over remnant of something that cannot collide using just a one loop collider. </p>
<p>Qubit</p>
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		<title>By: Q</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-107878</link>
		<dc:creator>Q</dc:creator>
		<pubDate>Sun, 30 Jul 2006 18:31:59 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-107878</guid>
		<description>Well JoAnne, seems most of the physicists are too busy jumping into the pool to 'cool' down or jumping onto planes to 'teleport' back to wherever they flew in from. Either that or they are at the races.

You should have offered some odds:
10-1 Condoleeza turns into a stable 'singularity'
10-2 Condoleeza turns into an unstable 'singulrity'
10-3 Condoleeza 'evaporates'

You might have got some more hard 'particle' physics.
Bee can Hans Stoker guy really take out a patent on Back to the Future movies. it's not a chevy - its a Delorean, and there weren't that many made. But wow if they'd got it to really work, would have been worth a mint.

&lt;strong&gt;Quote of the Day:&lt;/strong&gt; Prediction is very difficult, especially if it's about the future. Niels Bohr</description>
		<content:encoded><![CDATA[<p>Well JoAnne, seems most of the physicists are too busy jumping into the pool to &#8216;cool&#8217; down or jumping onto planes to &#8216;teleport&#8217; back to wherever they flew in from. Either that or they are at the races.</p>
<p>You should have offered some odds:<br />
10-1 Condoleeza turns into a stable &#8217;singularity&#8217;<br />
10-2 Condoleeza turns into an unstable &#8217;singulrity&#8217;<br />
10-3 Condoleeza &#8216;evaporates&#8217;</p>
<p>You might have got some more hard &#8216;particle&#8217; physics.<br />
Bee can Hans Stoker guy really take out a patent on Back to the Future movies. it&#8217;s not a chevy - its a Delorean, and there weren&#8217;t that many made. But wow if they&#8217;d got it to really work, would have been worth a mint.</p>
<p><strong>Quote of the Day:</strong> Prediction is very difficult, especially if it&#8217;s about the future. Niels Bohr</p>
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		<title>By: Tony Smith</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-107866</link>
		<dc:creator>Tony Smith</dc:creator>
		<pubDate>Sun, 30 Jul 2006 18:18:37 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-107866</guid>
		<description>B said "... How about this: the LHC reaches a fundamental minimal scale (the higher dimensional Planck length?) below which absolutely nothing more can be resolved, thus â€˜the end of short distance physicsâ€™. ...". 

JoAnne said that Condi mentioned LHC results "... indicative of noncommutative spacetime ...". 

If the LHC were to see a "higher dimensional Planck length" would that mean that phenomena of "noncommutative spacetime" should show up if Connes's model is correct ? 
What would be the experimental signatures of such "noncommutative spacetime" ?

Tony Smith
http://www.valdostamuseum.org/hamsmith/

PS - Why would anybody write "nasty comments" about hep-ph/0507138 by Bee et al ? 
What is wrong with using LHC to look for unusual stuff, whether or not it is unlikely ?</description>
		<content:encoded><![CDATA[<p>B said &#8220;&#8230; How about this: the LHC reaches a fundamental minimal scale (the higher dimensional Planck length?) below which absolutely nothing more can be resolved, thus â€˜the end of short distance physicsâ€™. &#8230;&#8221;. </p>
<p>JoAnne said that Condi mentioned LHC results &#8220;&#8230; indicative of noncommutative spacetime &#8230;&#8221;. </p>
<p>If the LHC were to see a &#8220;higher dimensional Planck length&#8221; would that mean that phenomena of &#8220;noncommutative spacetime&#8221; should show up if Connes&#8217;s model is correct ?<br />
What would be the experimental signatures of such &#8220;noncommutative spacetime&#8221; ?</p>
<p>Tony Smith<br />
<a href="http://www.valdostamuseum.org/hamsmith/" rel="nofollow">http://www.valdostamuseum.org/hamsmith/</a></p>
<p>PS - Why would anybody write &#8220;nasty comments&#8221; about hep-ph/0507138 by Bee et al ?<br />
What is wrong with using LHC to look for unusual stuff, whether or not it is unlikely ?</p>
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		<title>By: B</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-107863</link>
		<dc:creator>B</dc:creator>
		<pubDate>Sun, 30 Jul 2006 17:46:50 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-107863</guid>
		<description>well, Horst Stoecker is apparently holding a patent to use black hole remnants to convert mass into energy (&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607165" rel="nofollow"&gt;hep-ph/0607165, section 6)&lt;/a&gt;... think about this: the LHC produces all these remants, you put one in the back of your car, and feed it with - say, your empty Coke cans. Then it evaporate at 200 GeV, and boom there flies your Chevy.

Sorry, being silly here. You wouldn't believe how many nasty comments I got on my paper about signatures of &lt;a href="http://lanl.arxiv.org/abs/hep-ph/0507138" rel="nofollow"&gt;black hole remnants at the LHC&lt;/a&gt;. 

Anyway, I should add that I don't find the scenario plausible. My prediction is also the no-Higgs case, but then that's not surprising anymore. 

How about this: the LHC reaches a fundamental minimal scale (the higher dimensional Planck length?) below which absolutely nothing more can be resolved, thus 'the end of short distance physics'.

Best, B.</description>
		<content:encoded><![CDATA[<p>well, Horst Stoecker is apparently holding a patent to use black hole remnants to convert mass into energy (<a href="http://xxx.lanl.gov/abs/hep-ph/0607165" rel="nofollow">hep-ph/0607165, section 6)</a>&#8230; think about this: the LHC produces all these remants, you put one in the back of your car, and feed it with - say, your empty Coke cans. Then it evaporate at 200 GeV, and boom there flies your Chevy.</p>
<p>Sorry, being silly here. You wouldn&#8217;t believe how many nasty comments I got on my paper about signatures of <a href="http://lanl.arxiv.org/abs/hep-ph/0507138" rel="nofollow">black hole remnants at the LHC</a>. </p>
<p>Anyway, I should add that I don&#8217;t find the scenario plausible. My prediction is also the no-Higgs case, but then that&#8217;s not surprising anymore. </p>
<p>How about this: the LHC reaches a fundamental minimal scale (the higher dimensional Planck length?) below which absolutely nothing more can be resolved, thus &#8216;the end of short distance physics&#8217;.</p>
<p>Best, B.</p>
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		<title>By: scerir</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-107856</link>
		<dc:creator>scerir</dc:creator>
		<pubDate>Sun, 30 Jul 2006 16:34:55 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-107856</guid>
		<description>Which of the 'Drei Zinnen' (see pic on the panel) did the distinguished expert climb?</description>
		<content:encoded><![CDATA[<p>Which of the &#8216;Drei Zinnen&#8217; (see pic on the panel) did the distinguished expert climb?</p>
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		<title>By: bittergradstudent</title>
		<link>http://cosmicvariance.com/2006/07/28/most-surprising-lhc-discovery/#comment-107855</link>
		<dc:creator>bittergradstudent</dc:creator>
		<pubDate>Sun, 30 Jul 2006 16:32:45 +0000</pubDate>
		<guid isPermaLink="false">http://cosmicvariance.com/?p=927#comment-107855</guid>
		<description>Internal electron structure?</description>
		<content:encoded><![CDATA[<p>Internal electron structure?</p>
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