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	<title>Comments on: The Screwy Universe</title>
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	<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/</link>
	<description>Random samplings from a universe of ideas.</description>
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		<title>By: Thomas Dent</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16931</link>
		<dc:creator>Thomas Dent</dc:creator>
		<pubDate>Mon, 05 Jun 2006 22:53:30 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16931</guid>
		<description>Been travelling and missed most of the debate.

I still think &#039;smelling&#039; is bogus, and borders on insulting, given the careful work that has gone into the alpha and mu results. Some types of new physics are more fashionable than others, that&#039;s surely true, and the majority has the dubious privilege of saying that the 3.5 sigma deviations that the minority sometimes work on &#039;smell wrong&#039;. And the majority sometimes ends up working on the LEP so-called &#039;Higgs&#039;, or the muon magnetic moment, or CP asymmetries in B physics, all of which are (so far) not new physics either, by any sane definition.

Now most particle physicists are indeed looking towards LHC, which is a quite rational thing to do, but that doesn&#039;t mean Nature must be generous enough to give us a nice new discovery there. The thing is to be as prepared as possible for whatever is going to be thrown at us, which may come in the LHC, or somewhere completely different. Since the LHC will throw out a lotttt of data, simply by power of numbers it requires the most preparation.

There is simply no reason why anyone should place weight on a theorist&#039;s &#039;intuition&#039; about debatable experimental results. The only way to find out if such a result is right or wrong is - do more experiments.

&#039;Smelling&#039; and &#039;intuition&#039; about what are experimentally determinable facts are simply exhibitions of the theorist&#039;s prejudices. Naturally the theorist is sometimes right and sometimes wrong... then he can repeat the story of when he was right, and forget the times he was wrong.

Remember the muon - &#039;Who ordered that?&#039; The existence of three families is an awkward and messy fact that doesn&#039;t explain anything nicely, and caused a lot of theoretical problems, most of which are still unsolved. Three families smells terrible from almost every angle - but it is an experimental fact.

The cosmological constant also smells awful theoretically, with our current level of (lack of) understanding, unless you are prepared to accept some rather shaky anthropic type reasoning.

Now, it is not so much work to read up about how the alpha and mu results were obtained and what the possible problems with them actually are, then you might come to some sort of informed opinion, using the brain rather than the nose.

E.g. http://www.physik.uni-bielefeld.de/igs/schools/cosmology/cosmo-schedule.html for an elementary start.

Now to work.

Comparison of alpha and mu variations is very model dependent. The mu data are only at two redshifts and don&#039;t allow the drawing of any trend line. The alpha data don&#039;t show a clear trend although their average is significantly different from null. There is no pattern given present data. A linear variation with time (assuming that the value is spatially homogeneous) doesn&#039;t fit both Oklo and varying alpha. Neither does a linear variation with redshift. Anyway Oklo should be redone to take into account variation in nuclear physics parameters (not just alpha) but that is a mess because of nuclear physics being generally messy.

Thomas</description>
		<content:encoded><![CDATA[<p>Been travelling and missed most of the debate.</p>
<p>I still think &#8216;smelling&#8217; is bogus, and borders on insulting, given the careful work that has gone into the alpha and mu results. Some types of new physics are more fashionable than others, that&#8217;s surely true, and the majority has the dubious privilege of saying that the 3.5 sigma deviations that the minority sometimes work on &#8216;smell wrong&#8217;. And the majority sometimes ends up working on the LEP so-called &#8216;Higgs&#8217;, or the muon magnetic moment, or CP asymmetries in B physics, all of which are (so far) not new physics either, by any sane definition.</p>
<p>Now most particle physicists are indeed looking towards LHC, which is a quite rational thing to do, but that doesn&#8217;t mean Nature must be generous enough to give us a nice new discovery there. The thing is to be as prepared as possible for whatever is going to be thrown at us, which may come in the LHC, or somewhere completely different. Since the LHC will throw out a lotttt of data, simply by power of numbers it requires the most preparation.</p>
<p>There is simply no reason why anyone should place weight on a theorist&#8217;s &#8216;intuition&#8217; about debatable experimental results. The only way to find out if such a result is right or wrong is &#8211; do more experiments.</p>
<p>&#8216;Smelling&#8217; and &#8216;intuition&#8217; about what are experimentally determinable facts are simply exhibitions of the theorist&#8217;s prejudices. Naturally the theorist is sometimes right and sometimes wrong&#8230; then he can repeat the story of when he was right, and forget the times he was wrong.</p>
<p>Remember the muon &#8211; &#8216;Who ordered that?&#8217; The existence of three families is an awkward and messy fact that doesn&#8217;t explain anything nicely, and caused a lot of theoretical problems, most of which are still unsolved. Three families smells terrible from almost every angle &#8211; but it is an experimental fact.</p>
<p>The cosmological constant also smells awful theoretically, with our current level of (lack of) understanding, unless you are prepared to accept some rather shaky anthropic type reasoning.</p>
<p>Now, it is not so much work to read up about how the alpha and mu results were obtained and what the possible problems with them actually are, then you might come to some sort of informed opinion, using the brain rather than the nose.</p>
<p>E.g. <a href="http://www.physik.uni-bielefeld.de/igs/schools/cosmology/cosmo-schedule.html" rel="nofollow">http://www.physik.uni-bielefeld.de/igs/schools/cosmology/cosmo-schedule.html</a> for an elementary start.</p>
<p>Now to work.</p>
<p>Comparison of alpha and mu variations is very model dependent. The mu data are only at two redshifts and don&#8217;t allow the drawing of any trend line. The alpha data don&#8217;t show a clear trend although their average is significantly different from null. There is no pattern given present data. A linear variation with time (assuming that the value is spatially homogeneous) doesn&#8217;t fit both Oklo and varying alpha. Neither does a linear variation with redshift. Anyway Oklo should be redone to take into account variation in nuclear physics parameters (not just alpha) but that is a mess because of nuclear physics being generally messy.</p>
<p>Thomas</p>
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		<title>By: JoAnne</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16907</link>
		<dc:creator>JoAnne</dc:creator>
		<pubDate>Mon, 05 Jun 2006 05:53:28 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16907</guid>
		<description>Sean says:  &quot;It was the only time in my life when I worked feverishly over the course of a couple of days to write a paper from scratch.&quot;

Ah....that&#039;s what happens when there is DATA!!  Counting down desperately to the LHC....</description>
		<content:encoded><![CDATA[<p>Sean says:  &#8220;It was the only time in my life when I worked feverishly over the course of a couple of days to write a paper from scratch.&#8221;</p>
<p>Ah&#8230;.that&#8217;s what happens when there is DATA!!  Counting down desperately to the LHC&#8230;.</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16908</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Mon, 05 Jun 2006 04:47:46 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16908</guid>
		<description>The essence is that some people thought there was evidence for the universe having a handedness, but those people were not right.  (To be careful:  we&#039;ve known for some time that some particle interactions, specifically the weak nuclear force, definitely exhibit a handedness -- they violate parity.  But there is no evidence that space itself has any such property.)</description>
		<content:encoded><![CDATA[<p>The essence is that some people thought there was evidence for the universe having a handedness, but those people were not right.  (To be careful:  we&#8217;ve known for some time that some particle interactions, specifically the weak nuclear force, definitely exhibit a handedness &#8212; they violate parity.  But there is no evidence that space itself has any such property.)</p>
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		<title>By: g randy primm</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16930</link>
		<dc:creator>g randy primm</dc:creator>
		<pubDate>Mon, 05 Jun 2006 04:34:08 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16930</guid>
		<description>i&#039;m just an ignorant bystander, but i&#039;m going to open my big yap anyway:

if i understand this discussion at all, it may be the case that the universe has an inherent &quot;handedness.&quot;

what the cause may be is poorly understood (if at all), but this handedness exists, nonetheless.

is this the essence of the discussion?</description>
		<content:encoded><![CDATA[<p>i&#8217;m just an ignorant bystander, but i&#8217;m going to open my big yap anyway:</p>
<p>if i understand this discussion at all, it may be the case that the universe has an inherent &#8220;handedness.&#8221;</p>
<p>what the cause may be is poorly understood (if at all), but this handedness exists, nonetheless.</p>
<p>is this the essence of the discussion?</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16929</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Sun, 04 Jun 2006 16:17:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16929</guid>
		<description>Shantanu, it would imply Lorentz violation of some sort, which may or may not take the form of a vector field.  But more likely it&#039;s just not right; it seems hard to make it consistent with other experimental bounds.</description>
		<content:encoded><![CDATA[<p>Shantanu, it would imply Lorentz violation of some sort, which may or may not take the form of a vector field.  But more likely it&#8217;s just not right; it seems hard to make it consistent with other experimental bounds.</p>
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		<title>By: Shantanu</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16928</link>
		<dc:creator>Shantanu</dc:creator>
		<pubDate>Sun, 04 Jun 2006 04:08:50 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16928</guid>
		<description>Sean, if the results of &lt;a href=&quot;http://arxiv.org/abs/gr-qc/0511160&quot; rel=&quot;nofollow&quot;&gt;
this &lt;/a&gt; are true, would that imply  the existence of a vector field?</description>
		<content:encoded><![CDATA[<p>Sean, if the results of <a href="http://arxiv.org/abs/gr-qc/0511160" rel="nofollow"><br />
this </a> are true, would that imply  the existence of a vector field?</p>
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		<title>By: Subhendra Mohanty</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16927</link>
		<dc:creator>Subhendra Mohanty</dc:creator>
		<pubDate>Fri, 02 Jun 2006 14:12:23 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16927</guid>
		<description>Sean,
     Thanks for the reference. I checked  the citations of this paper to see if some-one actually has used the WMAP data for putting some bounds and found a recent paper ( astro-ph/0601095 - acccepted in PRL) in which they claim that there is a  signal(!)for a non-zero external vector field which couples to photons, from the WMAP+Boomerang data.</description>
		<content:encoded><![CDATA[<p>Sean,<br />
     Thanks for the reference. I checked  the citations of this paper to see if some-one actually has used the WMAP data for putting some bounds and found a recent paper ( astro-ph/0601095 &#8211; acccepted in PRL) in which they claim that there is a  signal(!)for a non-zero external vector field which couples to photons, from the WMAP+Boomerang data.</p>
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		<title>By: The Uninitiated</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16926</link>
		<dc:creator>The Uninitiated</dc:creator>
		<pubDate>Thu, 01 Jun 2006 21:51:49 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16926</guid>
		<description>I get it now.  Thanks for clarifying, Sean!  It&#039;s one of your great talents.</description>
		<content:encoded><![CDATA[<p>I get it now.  Thanks for clarifying, Sean!  It&#8217;s one of your great talents.</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16925</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Thu, 01 Jun 2006 21:47:54 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16925</guid>
		<description>Uninitiated, sure, the cosmological rest frame and the entropy gradient definitely do define a direction in spacetime, at least on average over large scales.  But that&#039;s due to the evolution of matter fields; I was imagining a vector that would exist even in vacuum.

Joshua, I haven&#039;t been following the debates closely, although I have talked a bit with Jacobson about this.  I also tend to worry about superluminal propagation, but someone needs to sit down and show what would actually go wrong.  I think Eugene is working on this, actually.</description>
		<content:encoded><![CDATA[<p>Uninitiated, sure, the cosmological rest frame and the entropy gradient definitely do define a direction in spacetime, at least on average over large scales.  But that&#8217;s due to the evolution of matter fields; I was imagining a vector that would exist even in vacuum.</p>
<p>Joshua, I haven&#8217;t been following the debates closely, although I have talked a bit with Jacobson about this.  I also tend to worry about superluminal propagation, but someone needs to sit down and show what would actually go wrong.  I think Eugene is working on this, actually.</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16924</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Thu, 01 Jun 2006 21:44:49 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16924</guid>
		<description>Subhendra, thanks for writing.  The CMB is certainly a promising place to look; but I doubt at this point that the limits are very good, just because the errors on the polarization angles are quite large.  (And the *distance* to the CMB isn&#039;t that much more than to a high-redshift galaxy, even if the redshift is much greater.)  I don&#039;t know if anyone has actually looked at the limits, but I know that people did anticipate the possibility:

http://arxiv.org/abs/astro-ph/9812088</description>
		<content:encoded><![CDATA[<p>Subhendra, thanks for writing.  The CMB is certainly a promising place to look; but I doubt at this point that the limits are very good, just because the errors on the polarization angles are quite large.  (And the *distance* to the CMB isn&#8217;t that much more than to a high-redshift galaxy, even if the redshift is much greater.)  I don&#8217;t know if anyone has actually looked at the limits, but I know that people did anticipate the possibility:</p>
<p><a href="http://arxiv.org/abs/astro-ph/9812088" rel="nofollow">http://arxiv.org/abs/astro-ph/9812088</a></p>
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		<title>By: Supernova</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16923</link>
		<dc:creator>Supernova</dc:creator>
		<pubDate>Thu, 01 Jun 2006 21:10:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16923</guid>
		<description>Sorry, for a moment there you did look a bit like an astronomer.  My mistake.  :P</description>
		<content:encoded><![CDATA[<p>Sorry, for a moment there you did look a bit like an astronomer.  My mistake.  <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_razz.gif' alt=':P' class='wp-smiley' /> </p>
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		<title>By: The Uninitiated</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16922</link>
		<dc:creator>The Uninitiated</dc:creator>
		<pubDate>Thu, 01 Jun 2006 17:13:56 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16922</guid>
		<description>Pardon the stupid question, but isn&#039;t there already a preferred timelike direction in spacetime, the one in which the universe is expanding and entropy is increasing?</description>
		<content:encoded><![CDATA[<p>Pardon the stupid question, but isn&#8217;t there already a preferred timelike direction in spacetime, the one in which the universe is expanding and entropy is increasing?</p>
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		<title>By: joshua</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16921</link>
		<dc:creator>joshua</dc:creator>
		<pubDate>Thu, 01 Jun 2006 17:06:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16921</guid>
		<description>Sean - There are definately many such models. My impression is that the new fields can generally be coupled only to gravity to avoid other very tight bounds. Our paper addressed specifically the so-called Einstein-Aether, or new Aether, theories but I am pretty sure that, unless finely tuned, any coupling to gravity would alter the dispersion relation of the graviton to give some subluminal mode that can be radiated in a Cerenkov process.

&lt;a href=&quot;http://arxiv.org/abs/gr-qc/0509083&quot; rel=&quot;nofollow&quot;&gt;Jacobson and Foster&lt;/a&gt; take this to mean that, in their &quot;ae-theory,&quot; the parameters should be chosen such that the effective graviton modes are all super-luminal. We discounted this possibility from the start, but I understand that some people are not so conventional.

Is that more clear? I am not really up on the current trends in spontaneous Lorentz breaking; are there any more plausable theories that you know of? Is superluminal propagation a very good out? I know its impossible to rule out, but I feel it is rather unattractive theoretically. Thanks.</description>
		<content:encoded><![CDATA[<p>Sean &#8211; There are definately many such models. My impression is that the new fields can generally be coupled only to gravity to avoid other very tight bounds. Our paper addressed specifically the so-called Einstein-Aether, or new Aether, theories but I am pretty sure that, unless finely tuned, any coupling to gravity would alter the dispersion relation of the graviton to give some subluminal mode that can be radiated in a Cerenkov process.</p>
<p><a href="http://arxiv.org/abs/gr-qc/0509083" rel="nofollow">Jacobson and Foster</a> take this to mean that, in their &#8220;ae-theory,&#8221; the parameters should be chosen such that the effective graviton modes are all super-luminal. We discounted this possibility from the start, but I understand that some people are not so conventional.</p>
<p>Is that more clear? I am not really up on the current trends in spontaneous Lorentz breaking; are there any more plausable theories that you know of? Is superluminal propagation a very good out? I know its impossible to rule out, but I feel it is rather unattractive theoretically. Thanks.</p>
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		<title>By: Subhendra Mohanty</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16920</link>
		<dc:creator>Subhendra Mohanty</dc:creator>
		<pubDate>Thu, 01 Jun 2006 17:05:30 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16920</guid>
		<description>Dear Sean,
          Your reminiscences in your blog about the Screwy Universe brought back
          some memories. I had been back in India after a PhD from
          Wisconsin and I had been floundering about for some new
          ideas (and a permanent job!) when I read your paper with
          Field and Jackiw. It led me (with a couple of graduate students) to write a paper on getting
          such a Chern-Simon type of term from one loop effects in QED with CP violation.
          We got a very kind referee (and I suspect it may have been
          you because among other mistakes he pointed out that we
          had spelled Carroll incorrectly in the reference) and
          ultimately it was published as a Rapid Comm paper in PRD.
          That was my first paper in the field of astro-particle
          particle physics -the field wwhich has supplied my meal tickets ever since.

          Reading your remarks about quintessence generating
          polarization I thought of an idea (which you may have
          already thought of and discarded). Generally you improve
          the bounds on such couplings when you have a long-baseline
          for the photon. Now the longest baseline that is available
          for observation is that traversed by CMB photons from the
          LSS to us. The baseline is of the order of the age of the
          universe. If there is some quintessence type field
          with pseudosclar coupling to photons then it will
          contribute to the polarizations of the CMB (on which there
          are good constraints from WMAP-3). So using the WMAP
          polarization results one would probably get the best
          bounds on these type of couplings...?

          Best wishes,
          Subhendra</description>
		<content:encoded><![CDATA[<p>Dear Sean,<br />
          Your reminiscences in your blog about the Screwy Universe brought back<br />
          some memories. I had been back in India after a PhD from<br />
          Wisconsin and I had been floundering about for some new<br />
          ideas (and a permanent job!) when I read your paper with<br />
          Field and Jackiw. It led me (with a couple of graduate students) to write a paper on getting<br />
          such a Chern-Simon type of term from one loop effects in QED with CP violation.<br />
          We got a very kind referee (and I suspect it may have been<br />
          you because among other mistakes he pointed out that we<br />
          had spelled Carroll incorrectly in the reference) and<br />
          ultimately it was published as a Rapid Comm paper in PRD.<br />
          That was my first paper in the field of astro-particle<br />
          particle physics -the field wwhich has supplied my meal tickets ever since.</p>
<p>          Reading your remarks about quintessence generating<br />
          polarization I thought of an idea (which you may have<br />
          already thought of and discarded). Generally you improve<br />
          the bounds on such couplings when you have a long-baseline<br />
          for the photon. Now the longest baseline that is available<br />
          for observation is that traversed by CMB photons from the<br />
          LSS to us. The baseline is of the order of the age of the<br />
          universe. If there is some quintessence type field<br />
          with pseudosclar coupling to photons then it will<br />
          contribute to the polarizations of the CMB (on which there<br />
          are good constraints from WMAP-3). So using the WMAP<br />
          polarization results one would probably get the best<br />
          bounds on these type of couplings&#8230;?</p>
<p>          Best wishes,<br />
          Subhendra</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16919</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Thu, 01 Jun 2006 13:50:17 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16919</guid>
		<description>Robert -- the cosmological constant was a surprise, but it smelled very right.  There were two competing groups, both highly competent, looking for precisely that effect, and the result solved several well-known problems at once.  Likewise, neutrino oscillations were something that many people suspected for years.

Joshua -- I think I also agree that only spontaneously-broken models of Lorentz violation make sense, but there are plenty of such models.  Unless I am misunderstanding what you mean.</description>
		<content:encoded><![CDATA[<p>Robert &#8212; the cosmological constant was a surprise, but it smelled very right.  There were two competing groups, both highly competent, looking for precisely that effect, and the result solved several well-known problems at once.  Likewise, neutrino oscillations were something that many people suspected for years.</p>
<p>Joshua &#8212; I think I also agree that only spontaneously-broken models of Lorentz violation make sense, but there are plenty of such models.  Unless I am misunderstanding what you mean.</p>
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		<title>By: Robert</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16918</link>
		<dc:creator>Robert</dc:creator>
		<pubDate>Thu, 01 Jun 2006 10:43:29 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16918</guid>
		<description>Just for the record: How did the positive cosmological constant smell when it was first seen in supernova data and what about neutrino oscillations?</description>
		<content:encoded><![CDATA[<p>Just for the record: How did the positive cosmological constant smell when it was first seen in supernova data and what about neutrino oscillations?</p>
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		<title>By: Joshua</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16906</link>
		<dc:creator>Joshua</dc:creator>
		<pubDate>Thu, 01 Jun 2006 02:52:51 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16906</guid>
		<description>Hi Sean.

In &lt;em&gt;my&lt;/em&gt; first publication, me, Horace Stoica and my supervisor Guy Moore &lt;a href=&quot;http://arxiv.org/abs/hep-ph/0505211&quot; rel=&quot;nofollow&quot;&gt;put some bounds&lt;/a&gt; on a class of spontaneous Lorentz violating vector-tensor theories that provide a cherenkov-type mechanism by which cosmic rays could cool off way too much on even galactic distance scales.

I think we assumed throughout that the vev of the vector field was time-like and I recall having some very good reason for doing so. Barring acausal dispersion relations (in the less than speed of light sense), we found that these theories were very tightly constrained.

I came away from that work distinctly sceptical of any Lorentz violating theories, since my impression was that the spontaneously broken models were really the only viable candidates. I&#039;ve been told in rather passionate prose that this is too short sighted, but no-one can &lt;em&gt;really&lt;/em&gt; tell me why. Any help?

Thanks.</description>
		<content:encoded><![CDATA[<p>Hi Sean.</p>
<p>In <em>my</em> first publication, me, Horace Stoica and my supervisor Guy Moore <a href="http://arxiv.org/abs/hep-ph/0505211" rel="nofollow">put some bounds</a> on a class of spontaneous Lorentz violating vector-tensor theories that provide a cherenkov-type mechanism by which cosmic rays could cool off way too much on even galactic distance scales.</p>
<p>I think we assumed throughout that the vev of the vector field was time-like and I recall having some very good reason for doing so. Barring acausal dispersion relations (in the less than speed of light sense), we found that these theories were very tightly constrained.</p>
<p>I came away from that work distinctly sceptical of any Lorentz violating theories, since my impression was that the spontaneously broken models were really the only viable candidates. I&#8217;ve been told in rather passionate prose that this is too short sighted, but no-one can <em>really</em> tell me why. Any help?</p>
<p>Thanks.</p>
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		<title>By: N. Peter Armitage</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16917</link>
		<dc:creator>N. Peter Armitage</dc:creator>
		<pubDate>Thu, 01 Jun 2006 00:15:42 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16917</guid>
		<description>&gt;Although it&#039;s a fascinating discovery if true, there&#039;s something that doesn&#039;t
&gt;quite smell right about it. So I hit on the idea of first posting about the idea of
&gt;physics claims not &quot;smelling&quot; right more generally.

Aaah, the sweet smell of &#039;rightness&#039;.  Like pornography, we can&#039;t define it but we know it when we ...errr... see it.

An undergrad advisor of mine &lt;a href=&quot;http://www.physics.rutgers.edu/~devlin/&quot; rel=&quot;nofollow&quot;&gt;Tom Devlin &lt;/a&gt;,  first pointed out such an effect to me, but maintained that it wasn&#039;t a smell, but a sound.  He called it the &quot;&#039;ring&#039; of rightness.&quot;  Here, we know it when we hear it.

It&#039;s probably also what we call physics intuition, and it really is amazing what a powerful force it can be.  Frequently I think I&#039;m right about something only to be later proved wrong, but when that &#039;ding&#039; goes off after a thought that first glimpse usually turn out to be correct in the end.</description>
		<content:encoded><![CDATA[<p>&gt;Although it&#8217;s a fascinating discovery if true, there&#8217;s something that doesn&#8217;t<br />
&gt;quite smell right about it. So I hit on the idea of first posting about the idea of<br />
&gt;physics claims not &#8220;smelling&#8221; right more generally.</p>
<p>Aaah, the sweet smell of &#8216;rightness&#8217;.  Like pornography, we can&#8217;t define it but we know it when we &#8230;errr&#8230; see it.</p>
<p>An undergrad advisor of mine <a href="http://www.physics.rutgers.edu/~devlin/" rel="nofollow">Tom Devlin </a>,  first pointed out such an effect to me, but maintained that it wasn&#8217;t a smell, but a sound.  He called it the &#8220;&#8216;ring&#8217; of rightness.&#8221;  Here, we know it when we hear it.</p>
<p>It&#8217;s probably also what we call physics intuition, and it really is amazing what a powerful force it can be.  Frequently I think I&#8217;m right about something only to be later proved wrong, but when that &#8216;ding&#8217; goes off after a thought that first glimpse usually turn out to be correct in the end.</p>
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		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16916</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Thu, 01 Jun 2006 00:06:20 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16916</guid>
		<description>The best limits on the variations of most constants over cosmological timescales comes from Big Bang nucleosynthesis.  It&#039;s very long ago (redshift of one billion, or when the universe was three minutes old), but the precision isn&#039;t great.  If the Fermi constant (i.e., the Higgs expectation value) were to be different during BBN, it would change the neutron/proton mass difference, and thus both the neutron lifetime and the equilibrium n/p ratio, as well as the nuclear binding energies.  You typically find that G_F and other constants must be within about 10% of their current values.  See for example:

http://arxiv.org/abs/astro-ph/0508378</description>
		<content:encoded><![CDATA[<p>The best limits on the variations of most constants over cosmological timescales comes from Big Bang nucleosynthesis.  It&#8217;s very long ago (redshift of one billion, or when the universe was three minutes old), but the precision isn&#8217;t great.  If the Fermi constant (i.e., the Higgs expectation value) were to be different during BBN, it would change the neutron/proton mass difference, and thus both the neutron lifetime and the equilibrium n/p ratio, as well as the nuclear binding energies.  You typically find that G_F and other constants must be within about 10% of their current values.  See for example:</p>
<p><a href="http://arxiv.org/abs/astro-ph/0508378" rel="nofollow">http://arxiv.org/abs/astro-ph/0508378</a></p>
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		<title>By: Count Iblis</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/comment-page-1/#comment-16915</link>
		<dc:creator>Count Iblis</dc:creator>
		<pubDate>Wed, 31 May 2006 23:28:49 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/05/31/the-screwy-universe/#comment-16915</guid>
		<description>Wouldn&#039;t a variation of Fermi&#039;s constant have an observable impact on distant supernovae?</description>
		<content:encoded><![CDATA[<p>Wouldn&#8217;t a variation of Fermi&#8217;s constant have an observable impact on distant supernovae?</p>
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