<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	xmlns:sy="http://purl.org/rss/1.0/modules/syndication/"
		>
<channel>
	<title>Comments on: News From The Front, II</title>
	<atom:link href="http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/</link>
	<description>Random samplings from a universe of ideas.</description>
	<lastBuildDate>Tue, 14 Feb 2012 12:59:54 +0000</lastBuildDate>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
	<generator>http://wordpress.org/?v=3.2.1</generator>
	<item>
		<title>By: At The Monastery &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5968</link>
		<dc:creator>At The Monastery &#124; Cosmic Variance</dc:creator>
		<pubDate>Thu, 06 Jul 2006 17:23:58 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5968</guid>
		<description>[...] The above example is a rare case -especially in higher dimensional or &#8220;critical&#8221; string theory- where an exact computation allows one to track the dynamics of the vacuum of string theory in an off-shell formulation. (It is possible in several cute toy models of non-critical strings in low dimensions, such as those I&#8217;ve described in other posts here and here). This is the sort of thing of which we need a lot more before we have believable control over statements about what non-supersymmetric vacua of string theory are really up to. Until we have control over these issues, we&#8217;ve got to be very careful about what we&#8217;re doing in this context, taking explorations of such vacua -and phenomenological conclusions which may be drawn from them- as interesting, but highly tentative. [...]</description>
		<content:encoded><![CDATA[<p>[...] The above example is a rare case -especially in higher dimensional or &#8220;critical&#8221; string theory- where an exact computation allows one to track the dynamics of the vacuum of string theory in an off-shell formulation. (It is possible in several cute toy models of non-critical strings in low dimensions, such as those I&#8217;ve described in other posts here and here). This is the sort of thing of which we need a lot more before we have believable control over statements about what non-supersymmetric vacua of string theory are really up to. Until we have control over these issues, we&#8217;ve got to be very careful about what we&#8217;re doing in this context, taking explorations of such vacua -and phenomenological conclusions which may be drawn from them- as interesting, but highly tentative. [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Pause for a Glass of Wine &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5967</link>
		<dc:creator>Pause for a Glass of Wine &#124; Cosmic Variance</dc:creator>
		<pubDate>Thu, 01 Dec 2005 03:39:36 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5967</guid>
		<description>[...] So today they started with (technical stuff coming up) examining the properties of a particular conformal minimal model - the Lee-Yang model- and I tested their conformal field theory knowledge by getting them to extract the scaling operator dimensions from the Kac table, and deducing various properties of the model from that&#8230;. critical exponents, non-unitarity, etc. Then they turned to the subject of KPZ scaling, looking at the properties of the partition function of a conformal field theory coupled now to fluctuating surfaces as opposed to fixed ones. After reflecting upon the critical exponents encountered there, they moved to the meat of the exam: solving a specific model using matrix models techniques. The matrix model allows you to actually do the sum over random surfaces explicitly (by discretising them first) and extract the KPZ behaviour (by taking a careful continuum limit) for a class of conformal models obtained by tuning to a critical point in the model and carrying out the famous &#8220;double scaling limit&#8221;, which I talked about briefly here. In the end, they get a result for the partition function of the model, and if they&#8217;ve done everything properly (I walk them through it), they see KPZ scaling and they discover that they&#8217;ve derived the model of the Lee-Yang model (from the first part of the exam) coupled to random surfaces. We&#8217;ve come full circle, and they learned how to explicitly solve one of these models on their own, and tune it too find the critical behaviour that defines the continuum limit, etc. (It was only a 90 minute exam, so my plan to have something on solitons (something else we did in the course) was dropped. There was enough computation to be done in the stuff I gave.) [...]</description>
		<content:encoded><![CDATA[<p>[...] So today they started with (technical stuff coming up) examining the properties of a particular conformal minimal model &#8211; the Lee-Yang model- and I tested their conformal field theory knowledge by getting them to extract the scaling operator dimensions from the Kac table, and deducing various properties of the model from that&#8230;. critical exponents, non-unitarity, etc. Then they turned to the subject of KPZ scaling, looking at the properties of the partition function of a conformal field theory coupled now to fluctuating surfaces as opposed to fixed ones. After reflecting upon the critical exponents encountered there, they moved to the meat of the exam: solving a specific model using matrix models techniques. The matrix model allows you to actually do the sum over random surfaces explicitly (by discretising them first) and extract the KPZ behaviour (by taking a careful continuum limit) for a class of conformal models obtained by tuning to a critical point in the model and carrying out the famous &#8220;double scaling limit&#8221;, which I talked about briefly here. In the end, they get a result for the partition function of the model, and if they&#8217;ve done everything properly (I walk them through it), they see KPZ scaling and they discover that they&#8217;ve derived the model of the Lee-Yang model (from the first part of the exam) coupled to random surfaces. We&#8217;ve come full circle, and they learned how to explicitly solve one of these models on their own, and tune it too find the critical behaviour that defines the continuum limit, etc. (It was only a 90 minute exam, so my plan to have something on solitons (something else we did in the course) was dropped. There was enough computation to be done in the stuff I gave.) [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: News From The Front, III &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5966</link>
		<dc:creator>News From The Front, III &#124; Cosmic Variance</dc:creator>
		<pubDate>Fri, 04 Nov 2005 20:36:06 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5966</guid>
		<description>[...] Ok, so last time, I told you a bit about the motivations for what I&#8217;ve been up to. Now I want to simply show you some of the product. I&#8217;m going to use pictures, words, and equations. I will lose some of you, and for that I&#8217;m sorry. But I hope that the words will still give you the gist of the thing. I&#8217;ll answer some of your questions in the comments. [...]</description>
		<content:encoded><![CDATA[<p>[...] Ok, so last time, I told you a bit about the motivations for what I&#8217;ve been up to. Now I want to simply show you some of the product. I&#8217;m going to use pictures, words, and equations. I will lose some of you, and for that I&#8217;m sorry. But I hope that the words will still give you the gist of the thing. I&#8217;ll answer some of your questions in the comments. [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Plato</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5965</link>
		<dc:creator>Plato</dc:creator>
		<pubDate>Wed, 02 Nov 2005 03:40:22 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5965</guid>
		<description>Well, I like the reference to the simple experiments of the pendulum, but &lt;a href=&quot;http://eskesthai.blogspot.com/2005/11/harmonic-oscillation.html&quot; rel=&quot;nofollow&quot;&gt;this can be taken further&lt;/a&gt;?</description>
		<content:encoded><![CDATA[<p>Well, I like the reference to the simple experiments of the pendulum, but <a href="http://eskesthai.blogspot.com/2005/11/harmonic-oscillation.html" rel="nofollow">this can be taken further</a>?</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Wolfgang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5964</link>
		<dc:creator>Wolfgang</dc:creator>
		<pubDate>Wed, 02 Nov 2005 00:35:10 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5964</guid>
		<description>Clifford,

the hydrogen atom is certainly not  a &quot;toy model&quot;.  The other examples you mention are important as long as they neglect the &quot;minor details&quot; only.
But feel free to call you model(s) whatever you like. They are certainly very important, otherwise you would not analyze them.</description>
		<content:encoded><![CDATA[<p>Clifford,</p>
<p>the hydrogen atom is certainly not  a &#8220;toy model&#8221;.  The other examples you mention are important as long as they neglect the &#8220;minor details&#8221; only.<br />
But feel free to call you model(s) whatever you like. They are certainly very important, otherwise you would not analyze them.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Clifford</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5963</link>
		<dc:creator>Clifford</dc:creator>
		<pubDate>Wed, 02 Nov 2005 00:16:30 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5963</guid>
		<description>Pyracantha....that&#039;s ok. Don&#039;t fall into the common trap that people do in thinking that if they do not get it really quickly then it is either hard, confusing, or not well explained. This is a lot of the origin of people not &quot;getting&quot; science. They don&#039;t realise that you have to work at it a bit. Things that are worth understanding often take time to digest. I did not intend for you to understand the pendulum -or nonperturbative string theory- all in one go if you&#039;ve never studied it before. Take what I said (which was a bit rough and ready, admittedly) and put it alongside a proper book on the subject.

Take the time....it is worth it.

Cheers,

-cvj</description>
		<content:encoded><![CDATA[<p>Pyracantha&#8230;.that&#8217;s ok. Don&#8217;t fall into the common trap that people do in thinking that if they do not get it really quickly then it is either hard, confusing, or not well explained. This is a lot of the origin of people not &#8220;getting&#8221; science. They don&#8217;t realise that you have to work at it a bit. Things that are worth understanding often take time to digest. I did not intend for you to understand the pendulum -or nonperturbative string theory- all in one go if you&#8217;ve never studied it before. Take what I said (which was a bit rough and ready, admittedly) and put it alongside a proper book on the subject.</p>
<p>Take the time&#8230;.it is worth it.</p>
<p>Cheers,</p>
<p>-cvj</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Clifford</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5962</link>
		<dc:creator>Clifford</dc:creator>
		<pubDate>Wed, 02 Nov 2005 00:12:29 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5962</guid>
		<description>Wolfgang: &quot;toy model&quot;.... ah yes, I was waiting for that polite euphemism people use to pour scorn on a piece of physics because it suffers from the affliction of being a tractable problem. We&#039;re only supposed to care about the stuff we can&#039;t make any progress in, I suppose. Well, fine. But I will remind you that the harmonic oscillator, the Ising model, the hydrogen atom, and a host of other &quot;toy models&quot; form the foundation of what we really know and truly understand about many diverse areas of physics.

Cheers,


-cvj</description>
		<content:encoded><![CDATA[<p>Wolfgang: &#8220;toy model&#8221;&#8230;. ah yes, I was waiting for that polite euphemism people use to pour scorn on a piece of physics because it suffers from the affliction of being a tractable problem. We&#8217;re only supposed to care about the stuff we can&#8217;t make any progress in, I suppose. Well, fine. But I will remind you that the harmonic oscillator, the Ising model, the hydrogen atom, and a host of other &#8220;toy models&#8221; form the foundation of what we really know and truly understand about many diverse areas of physics.</p>
<p>Cheers,</p>
<p>-cvj</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Pyracantha</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5961</link>
		<dc:creator>Pyracantha</dc:creator>
		<pubDate>Wed, 02 Nov 2005 00:04:56 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5961</guid>
		<description>Clifford:

      Sorry to say this, but you lost me after the first paragraph. I will print your reply out and save it until I am able to understand it, which may be a few years from now. I have not studied pendulum motion yet. I am still trying to fathom F=ma and sliding blocks, let alone Newton&#039;s law of universal gravity. I am a real slow student.</description>
		<content:encoded><![CDATA[<p>Clifford:</p>
<p>      Sorry to say this, but you lost me after the first paragraph. I will print your reply out and save it until I am able to understand it, which may be a few years from now. I have not studied pendulum motion yet. I am still trying to fathom F=ma and sliding blocks, let alone Newton&#8217;s law of universal gravity. I am a real slow student.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Today&#8217;s Faux pas &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5960</link>
		<dc:creator>Today&#8217;s Faux pas &#124; Cosmic Variance</dc:creator>
		<pubDate>Tue, 01 Nov 2005 23:36:25 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5960</guid>
		<description>[...] So it has been one of those weeks so far, where my inexperience about things at USC have tripped up my good intentions and let to some excruciatingly embarrassing screwups. Yesterday, I was supposed to be at a big two hour lunch meeting at the Annenberg Center for Communication where we (lots of the great and the good of the Los Angeles &#8220;learned&#8221; folk -plus me-) brainstormed about Science and Creativity. I get invited to take part in these things and I want to contribute, and it&#8217;s an honour, etc&#8230;&#8230; but I screwed up and did not make it, for reasons I described earlier. (Who knew there was both an Annenberg Center for Communications and an Annenberg School for Communications?) [...]</description>
		<content:encoded><![CDATA[<p>[...] So it has been one of those weeks so far, where my inexperience about things at USC have tripped up my good intentions and let to some excruciatingly embarrassing screwups. Yesterday, I was supposed to be at a big two hour lunch meeting at the Annenberg Center for Communication where we (lots of the great and the good of the Los Angeles &#8220;learned&#8221; folk -plus me-) brainstormed about Science and Creativity. I get invited to take part in these things and I want to contribute, and it&#8217;s an honour, etc&#8230;&#8230; but I screwed up and did not make it, for reasons I described earlier. (Who knew there was both an Annenberg Center for Communications and an Annenberg School for Communications?) [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Wolfgang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5959</link>
		<dc:creator>Wolfgang</dc:creator>
		<pubDate>Tue, 01 Nov 2005 22:27:10 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5959</guid>
		<description>Anonymous,

Jacques wrote a nice post about the subcritical model you mention,
several years ago
http://golem.ph.utexas.edu/~distler/blog/archives/000206.html

Interesting indeed, but can we agree that this falls in the category of &quot;toy model&quot; ?</description>
		<content:encoded><![CDATA[<p>Anonymous,</p>
<p>Jacques wrote a nice post about the subcritical model you mention,<br />
several years ago<br />
<a href="http://golem.ph.utexas.edu/~distler/blog/archives/000206.html" rel="nofollow">http://golem.ph.utexas.edu/~distler/blog/archives/000206.html</a></p>
<p>Interesting indeed, but can we agree that this falls in the category of &#8220;toy model&#8221; ?</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Clifford</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5958</link>
		<dc:creator>Clifford</dc:creator>
		<pubDate>Tue, 01 Nov 2005 22:19:21 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5958</guid>
		<description>Anonymous.... you&#039;ve answered all the points for me. Thanks.  That was very helpful. I have not read any of the discussion of the stuff on those other blogs, and so could not comment on their content.

I was busy with other things, not ignoring you Wolfgang. I did not mean my short reply to be a slap in the face, which is how you seem to have taken it....It&#039;s just that I have this job I get paid for and it takes me away from blogging from time to time so my answers are not always as immediate, long (or existent) as at other times!

Cheers!

-cvj</description>
		<content:encoded><![CDATA[<p>Anonymous&#8230;. you&#8217;ve answered all the points for me. Thanks.  That was very helpful. I have not read any of the discussion of the stuff on those other blogs, and so could not comment on their content.</p>
<p>I was busy with other things, not ignoring you Wolfgang. I did not mean my short reply to be a slap in the face, which is how you seem to have taken it&#8230;.It&#8217;s just that I have this job I get paid for and it takes me away from blogging from time to time so my answers are not always as immediate, long (or existent) as at other times!</p>
<p>Cheers!</p>
<p>-cvj</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Anonymous</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5957</link>
		<dc:creator>Anonymous</dc:creator>
		<pubDate>Tue, 01 Nov 2005 20:53:52 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5957</guid>
		<description>Wolfgang, note that Jacques also mentions the 2-d &lt;i&gt;sub&lt;/i&gt;critical string:

&quot;In 1+1 dimensional noncritical string theory, there is also a linear dilaton background (varying in a spacelike direction). And there&#039;s a &quot;Tachyon wall,&quot; preventing strings from penetrating the region of strong coupling. So one has an S-matrix, of sorts, for string coming in from the weakly-coupled region, bouncing off the wall, and returning to the weakly-coupled region.&quot;

See? In that case you do have some notion of an S-matrix.</description>
		<content:encoded><![CDATA[<p>Wolfgang, note that Jacques also mentions the 2-d <i>sub</i>critical string:</p>
<p>&#8220;In 1+1 dimensional noncritical string theory, there is also a linear dilaton background (varying in a spacelike direction). And there&#8217;s a &#8220;Tachyon wall,&#8221; preventing strings from penetrating the region of strong coupling. So one has an S-matrix, of sorts, for string coming in from the weakly-coupled region, bouncing off the wall, and returning to the weakly-coupled region.&#8221;</p>
<p>See? In that case you do have some notion of an S-matrix.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Wolfgang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5956</link>
		<dc:creator>Wolfgang</dc:creator>
		<pubDate>Tue, 01 Nov 2005 20:00:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5956</guid>
		<description>Anonymous,

Jacques points out what the problem is with super-critical models using a linear dilatons in the post you link to:
&quot;However, for supercritical strings, the theory is strongly-coupled either in the far future or in the far past. It&#039;s not clear how one defines an S-matrix.&quot;

Again, at this point I assume that I have completely misunderstood what Clifford
is doing, since he certainly knows all this much better than I do (by a factor of many gogols 8-) .</description>
		<content:encoded><![CDATA[<p>Anonymous,</p>
<p>Jacques points out what the problem is with super-critical models using a linear dilatons in the post you link to:<br />
&#8220;However, for supercritical strings, the theory is strongly-coupled either in the far future or in the far past. It&#8217;s not clear how one defines an S-matrix.&#8221;</p>
<p>Again, at this point I assume that I have completely misunderstood what Clifford<br />
is doing, since he certainly knows all this much better than I do (by a factor of many gogols <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_cool.gif' alt='8-)' class='wp-smiley' /> .</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Anonymous</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5955</link>
		<dc:creator>Anonymous</dc:creator>
		<pubDate>Tue, 01 Nov 2005 19:03:41 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5955</guid>
		<description>Wolfgang, the important thing is that the CFT have the right central charge. There are plenty of CFTs around that can do this, aside from the usual flat target space with constant dilaton. A well-known example is the linear dilaton.

If you&#039;re looking at old blog posts, you should see one by Jacques Distler, http://golem.ph.utexas.edu/~distler/blog/archives/000551.html.

The low-dimensional noncritical string theories are not controversial in the way the supercritical ones are. Give Clifford some credit.</description>
		<content:encoded><![CDATA[<p>Wolfgang, the important thing is that the CFT have the right central charge. There are plenty of CFTs around that can do this, aside from the usual flat target space with constant dilaton. A well-known example is the linear dilaton.</p>
<p>If you&#8217;re looking at old blog posts, you should see one by Jacques Distler, <a href="http://golem.ph.utexas.edu/~distler/blog/archives/000551.html" rel="nofollow">http://golem.ph.utexas.edu/~distler/blog/archives/000551.html</a>.</p>
<p>The low-dimensional noncritical string theories are not controversial in the way the supercritical ones are. Give Clifford some credit.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Wolfgang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5954</link>
		<dc:creator>Wolfgang</dc:creator>
		<pubDate>Tue, 01 Nov 2005 18:36:38 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5954</guid>
		<description>I am even too stupid to use a keyboard:
Gouis = Gomis and amy = may in my previous post.</description>
		<content:encoded><![CDATA[<p>I am even too stupid to use a keyboard:<br />
Gouis = Gomis and amy = may in my previous post.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Wolfgang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5953</link>
		<dc:creator>Wolfgang</dc:creator>
		<pubDate>Tue, 01 Nov 2005 17:57:48 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5953</guid>
		<description>&gt; I beleive we&#039;re not talking about the same thing. There are no anomalies.

I assume that I am just too stupid to understand what your are talking about.
The little I know is that cancellation of anomalies requires D=10 for superstrings
(and D=11 for M-theory).
In non-critical string theories one can construct some clever ways to cancel the anomalies with higher order corrections a la Eva Silverstein and I think Jaume Gouis found another construction.
But these methods appear unphysical (see Lubos&#039; comments).

But I amy have completely misunderstood your post, especially the part
&gt; What people never tell you is that it is a complete overstatement to say that
&gt; string theory can only live in 10 dimensions. This is just wrong.</description>
		<content:encoded><![CDATA[<p>&gt; I beleive we&#8217;re not talking about the same thing. There are no anomalies.</p>
<p>I assume that I am just too stupid to understand what your are talking about.<br />
The little I know is that cancellation of anomalies requires D=10 for superstrings<br />
(and D=11 for M-theory).<br />
In non-critical string theories one can construct some clever ways to cancel the anomalies with higher order corrections a la Eva Silverstein and I think Jaume Gouis found another construction.<br />
But these methods appear unphysical (see Lubos&#8217; comments).</p>
<p>But I amy have completely misunderstood your post, especially the part<br />
&gt; What people never tell you is that it is a complete overstatement to say that<br />
&gt; string theory can only live in 10 dimensions. This is just wrong.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Clifford</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5952</link>
		<dc:creator>Clifford</dc:creator>
		<pubDate>Tue, 01 Nov 2005 17:21:02 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5952</guid>
		<description>I beleive we&#039;re not talking about the same thing. There are no anomalies.

-cvj</description>
		<content:encoded><![CDATA[<p>I beleive we&#8217;re not talking about the same thing. There are no anomalies.</p>
<p>-cvj</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Wolfgang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5951</link>
		<dc:creator>Wolfgang</dc:creator>
		<pubDate>Tue, 01 Nov 2005 17:11:55 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5951</guid>
		<description>&gt; I&#039;ve not too much interest in discussing the existence of other discussions on other physics on other blogs.

Sure. Well, you will have to deal with (or explain away) the anomalies and the way I see it, the case for super-symmetry is mostly gone.
It is a different story, of course, if you consider non-critical strings as toy models only.

I wish you good luck of course.</description>
		<content:encoded><![CDATA[<p>&gt; I&#8217;ve not too much interest in discussing the existence of other discussions on other physics on other blogs.</p>
<p>Sure. Well, you will have to deal with (or explain away) the anomalies and the way I see it, the case for super-symmetry is mostly gone.<br />
It is a different story, of course, if you consider non-critical strings as toy models only.</p>
<p>I wish you good luck of course.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Clifford</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5950</link>
		<dc:creator>Clifford</dc:creator>
		<pubDate>Tue, 01 Nov 2005 17:00:35 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5950</guid>
		<description>Yeah, I know it&#039;s different. Thanks. This is subcritical..... but in any case, I assume that Wolfgang was joking....making contact with interesting physics is a good thing, irrespective of who one might have to argue with.

So how about we talk about physics now, folks? I&#039;ve not too much interest in discussing the existence of other discussions on other physics on other blogs.

Cheers,

-cvj</description>
		<content:encoded><![CDATA[<p>Yeah, I know it&#8217;s different. Thanks. This is subcritical&#8230;.. but in any case, I assume that Wolfgang was joking&#8230;.making contact with interesting physics is a good thing, irrespective of who one might have to argue with.</p>
<p>So how about we talk about physics now, folks? I&#8217;ve not too much interest in discussing the existence of other discussions on other physics on other blogs.</p>
<p>Cheers,</p>
<p>-cvj</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Moshe</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/comment-page-1/#comment-5949</link>
		<dc:creator>Moshe</dc:creator>
		<pubDate>Tue, 01 Nov 2005 16:42:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2005/10/31/news-from-the-front-ii/#comment-5949</guid>
		<description>Clifford, Lubos had an exchange with Eva on his blog a while back in which he was critical of her work on super-critical strings, raising the issue of calculational control over these backgrounds. This is different from the non-critical strings you are discussing.</description>
		<content:encoded><![CDATA[<p>Clifford, Lubos had an exchange with Eva on his blog a while back in which he was critical of her work on super-critical strings, raising the issue of calculational control over these backgrounds. This is different from the non-critical strings you are discussing.</p>
]]></content:encoded>
	</item>
</channel>
</rss>

<!-- Performance optimized by W3 Total Cache. Learn more: http://www.w3-edge.com/wordpress-plugins/

Minified using disk
Page Caching using disk

Served from: blogs.discovermagazine.com @ 2012-02-14 13:00:28 -->
