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	<title>Comments on: 254A, Notes 3b: Brownian motion and Dyson Brownian motion</title>
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	<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/</link>
	<description>Updates on my research and expository papers, discussion of open problems, and other maths-related topics.  By Terence Tao</description>
	<lastBuildDate>Mon, 20 May 2013 01:46:06 +0000</lastBuildDate>
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	<item>
		<title>By: The Harish-Chandra-Itzykson-Zuber integral formula &#171; What&#8217;s new</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-216233</link>
		<dc:creator><![CDATA[The Harish-Chandra-Itzykson-Zuber integral formula &#171; What&#8217;s new]]></dc:creator>
		<pubDate>Sat, 09 Feb 2013 01:47:45 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-216233</guid>
		<description><![CDATA[[...] motion (as well as the closely related formulae for the GUE ensemble), which were derived in this previous blog post. Both of these approaches can be found in several places in the literature (and I do not actually [...]]]></description>
		<content:encoded><![CDATA[<p>[...] motion (as well as the closely related formulae for the GUE ensemble), which were derived in this previous blog post. Both of these approaches can be found in several places in the literature (and I do not actually [...]</p>
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	<item>
		<title>By: Some notes on Bakry-Emery theory &#171; What&#8217;s new</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-215889</link>
		<dc:creator><![CDATA[Some notes on Bakry-Emery theory &#171; What&#8217;s new]]></dc:creator>
		<pubDate>Tue, 05 Feb 2013 22:47:21 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-215889</guid>
		<description><![CDATA[[...]  is a stochastic process with initial probability distribution ; see for instance this previous blog post for more [...]]]></description>
		<content:encoded><![CDATA[<p>[...]  is a stochastic process with initial probability distribution ; see for instance this previous blog post for more [...]</p>
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		<title>By: hera</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-215672</link>
		<dc:creator><![CDATA[hera]]></dc:creator>
		<pubDate>Mon, 04 Feb 2013 10:10:07 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-215672</guid>
		<description><![CDATA[Great lecture! Prof. Tao, do you have ideas to simulate the Dyson&#039;s brownian motion ? I&#039;d like to do a computer simulation with MATLAB, can you give me some ideas?]]></description>
		<content:encoded><![CDATA[<p>Great lecture! Prof. Tao, do you have ideas to simulate the Dyson&#8217;s brownian motion ? I&#8217;d like to do a computer simulation with MATLAB, can you give me some ideas?</p>
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		<title>By: A direct proof of the stationarity of the Dyson sine process under Dyson Brownian motion &#171; What&#8217;s new</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-191739</link>
		<dc:creator><![CDATA[A direct proof of the stationarity of the Dyson sine process under Dyson Brownian motion &#171; What&#8217;s new]]></dc:creator>
		<pubDate>Sun, 11 Nov 2012 21:09:44 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-191739</guid>
		<description><![CDATA[[...] of a Hermitian matrix under independent Brownian motion of its entries, and is discussed in this previous blog post. To cut a long story short, this stationarity tells us that the self-similar -point correlation [...]]]></description>
		<content:encoded><![CDATA[<p>[...] of a Hermitian matrix under independent Brownian motion of its entries, and is discussed in this previous blog post. To cut a long story short, this stationarity tells us that the self-similar -point correlation [...]</p>
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	<item>
		<title>By: alabair</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-141176</link>
		<dc:creator><![CDATA[alabair]]></dc:creator>
		<pubDate>Tue, 01 May 2012 18:52:23 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-141176</guid>
		<description><![CDATA[I am amazed  by the surprising number of knowledge that is difficult to me to  digest. And by the way,  I would like to hear about a white noise process. Good luck.]]></description>
		<content:encoded><![CDATA[<p>I am amazed  by the surprising number of knowledge that is difficult to me to  digest. And by the way,  I would like to hear about a white noise process. Good luck.</p>
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	</item>
	<item>
		<title>By: Terence Tao</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-123384</link>
		<dc:creator><![CDATA[Terence Tao]]></dc:creator>
		<pubDate>Thu, 19 Jan 2012 02:09:41 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-123384</guid>
		<description><![CDATA[One can restore the confining potential by adding a $latex - \lambda_i dt$ term to the equation for $latex d\lambda_i$, turning the Dyson Brownian motion to a Dyson Ornstein-Uhlenbeck process.  This has the effect of keeping the variance of the matrix entries in the process constant, instead of growing linearly in time as is done here.  

The two processes (normalised variance and non-normalised variance) can be easily rescaled to each other, so the choice of which one to use is basically a matter of taste.]]></description>
		<content:encoded><![CDATA[<p>One can restore the confining potential by adding a <img src='http://s0.wp.com/latex.php?latex=-+%5Clambda_i+dt&amp;bg=ffffff&amp;fg=545454&amp;s=0' alt='- &#92;lambda_i dt' title='- &#92;lambda_i dt' class='latex' /> term to the equation for <img src='http://s0.wp.com/latex.php?latex=d%5Clambda_i&amp;bg=ffffff&amp;fg=545454&amp;s=0' alt='d&#92;lambda_i' title='d&#92;lambda_i' class='latex' />, turning the Dyson Brownian motion to a Dyson Ornstein-Uhlenbeck process.  This has the effect of keeping the variance of the matrix entries in the process constant, instead of growing linearly in time as is done here.  </p>
<p>The two processes (normalised variance and non-normalised variance) can be easily rescaled to each other, so the choice of which one to use is basically a matter of taste.</p>
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	<item>
		<title>By: Anonymous</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-123310</link>
		<dc:creator><![CDATA[Anonymous]]></dc:creator>
		<pubDate>Wed, 18 Jan 2012 20:12:21 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-123310</guid>
		<description><![CDATA[Hi prof. Tau, 

Thanks for these great notes! 

Maybe this question is much too late, but I&#039;d be very grateful for a reply. I&#039;m used to think about the eigenvalues of the GUE as being subjected to a quadratic confining potential and mutual log repulsion: is there an easy way to understand the absence of the effect of the confining potential (which would give rise to a simple harmonic restoring force for each eigenvalue) in the formula for the Dyson Brownian motion, equation (5)?

Thanks for a great blog!]]></description>
		<content:encoded><![CDATA[<p>Hi prof. Tau, </p>
<p>Thanks for these great notes! </p>
<p>Maybe this question is much too late, but I&#8217;d be very grateful for a reply. I&#8217;m used to think about the eigenvalues of the GUE as being subjected to a quadratic confining potential and mutual log repulsion: is there an easy way to understand the absence of the effect of the confining potential (which would give rise to a simple harmonic restoring force for each eigenvalue) in the formula for the Dyson Brownian motion, equation (5)?</p>
<p>Thanks for a great blog!</p>
]]></content:encoded>
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	<item>
		<title>By: Diffusion in Ehrenfest wind-tree model &#171; Disquisitiones Mathematicae</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-107227</link>
		<dc:creator><![CDATA[Diffusion in Ehrenfest wind-tree model &#171; Disquisitiones Mathematicae]]></dc:creator>
		<pubDate>Fri, 18 Nov 2011 10:38:03 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-107227</guid>
		<description><![CDATA[[...] the &#8220;justification&#8221; of the word &#8220;abnormal&#8221; comes by comparison with Brownian motion and/or central limit theorem: once we know that the diffusion is &#8220;sublinear&#8221; (maybe [...]]]></description>
		<content:encoded><![CDATA[<p>[...] the &#8220;justification&#8221; of the word &#8220;abnormal&#8221; comes by comparison with Brownian motion and/or central limit theorem: once we know that the diffusion is &#8220;sublinear&#8221; (maybe [...]</p>
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	</item>
	<item>
		<title>By: On Understanding Probability Puzzles &#124; Nair Research Notes</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-69252</link>
		<dc:creator><![CDATA[On Understanding Probability Puzzles &#124; Nair Research Notes]]></dc:creator>
		<pubDate>Sun, 21 Aug 2011 17:36:23 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-69252</guid>
		<description><![CDATA[[...] by , from an experimental point of view. The formal construction for the Brownian motion can be found here for example. And you will get a good historical perspective of the Brownian motion here. One of the [...]]]></description>
		<content:encoded><![CDATA[<p>[...] by , from an experimental point of view. The formal construction for the Brownian motion can be found here for example. And you will get a good historical perspective of the Brownian motion here. One of the [...]</p>
]]></content:encoded>
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	<item>
		<title>By: Dyson Brownian Motion &#124; Research Notebook</title>
		<link>http://terrytao.wordpress.com/2010/01/18/254a-notes-3b-brownian-motion-and-dyson-brownian-motion/#comment-57221</link>
		<dc:creator><![CDATA[Dyson Brownian Motion &#124; Research Notebook]]></dc:creator>
		<pubDate>Fri, 15 Jul 2011 17:59:28 +0000</pubDate>
		<guid isPermaLink="false">http://terrytao.wordpress.com/?p=3363#comment-57221</guid>
		<description><![CDATA[[...] main source for the material in this post is Terry Tao&#8216;s set of lecture notes on Random Matrix Theory, though I also used Mehta (2004) and Anderson, Guinnet and Zeitouni (2009) as [...]]]></description>
		<content:encoded><![CDATA[<p>[...] main source for the material in this post is Terry Tao&#8216;s set of lecture notes on Random Matrix Theory, though I also used Mehta (2004) and Anderson, Guinnet and Zeitouni (2009) as [...]</p>
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