<?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: WMAP 5-Year Results Released</title>
	<atom:link href="http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/</link>
	<description>Random samplings from a universe of ideas.</description>
	<lastBuildDate>Mon, 09 Nov 2009 11:26:47 -0600</lastBuildDate>
	<generator>http://wordpress.org/?v=2.8.4</generator>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
		<item>
		<title>By: Dipolo CMbr: acelerando a través del Universo &#124; Imagen astronomía diaria - Observatorio</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-93919</link>
		<dc:creator>Dipolo CMbr: acelerando a través del Universo &#124; Imagen astronomía diaria - Observatorio</dc:creator>
		<pubDate>Sun, 06 Sep 2009 06:01:28 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-93919</guid>
		<description>[...] del movimiento de la Tierra aparece corrida al azul y por tanto más caliente, mientras que la radiación del lado opuesto del cielo está corrida al rojo y más fría. El mapa indica que el Grupo Local se [...]</description>
		<content:encoded><![CDATA[<p>[...] del movimiento de la Tierra aparece corrida al azul y por tanto más caliente, mientras que la radiación del lado opuesto del cielo está corrida al rojo y más fría. El mapa indica que el Grupo Local se [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: A Special Place in the Universe &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37876</link>
		<dc:creator>A Special Place in the Universe &#124; Cosmic Variance</dc:creator>
		<pubDate>Fri, 07 Nov 2008 19:51:26 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37876</guid>
		<description>[...] now we have some predictions to compare with data, so that we can understand exactly how well the cosmic microwave background really assures us that there is no special place in the universe. But aside from the general [...]</description>
		<content:encoded><![CDATA[<p>[...] now we have some predictions to compare with data, so that we can understand exactly how well the cosmic microwave background really assures us that there is no special place in the universe. But aside from the general [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: WMAP 5-YEARS</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37874</link>
		<dc:creator>WMAP 5-YEARS</dc:creator>
		<pubDate>Sat, 02 Aug 2008 21:03:12 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37874</guid>
		<description>[...] clipped from cosmicvariance.com [...]</description>
		<content:encoded><![CDATA[<p>[...] clipped from cosmicvariance.com [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: The Lopsided Universe &#124; Cosmic Variance</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37875</link>
		<dc:creator>The Lopsided Universe &#124; Cosmic Variance</dc:creator>
		<pubDate>Sun, 08 Jun 2008 19:55:54 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37875</guid>
		<description>[...] collaborators: it&#8217;s lopsided. We all (all my friends, anyway) have seen the pretty pictures from the WMAP satellite, showing the 1-part-in-100,000 fluctuations in the temperature of the CMB from place to place in [...]</description>
		<content:encoded><![CDATA[<p>[...] collaborators: it&#8217;s lopsided. We all (all my friends, anyway) have seen the pretty pictures from the WMAP satellite, showing the 1-part-in-100,000 fluctuations in the temperature of the CMB from place to place in [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: John Merryman</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37873</link>
		<dc:creator>John Merryman</dc:creator>
		<pubDate>Wed, 12 Mar 2008 00:57:35 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37873</guid>
		<description>Lawrence,

If time is a measurement, than what physically exists is perfectly conserved, as it passes from one macro-state to the next. It is only these macro states that are created and consumed.</description>
		<content:encoded><![CDATA[<p>Lawrence,</p>
<p>If time is a measurement, than what physically exists is perfectly conserved, as it passes from one macro-state to the next. It is only these macro states that are created and consumed.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Lawrence B. Crowell</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37872</link>
		<dc:creator>Lawrence B. Crowell</dc:creator>
		<pubDate>Tue, 11 Mar 2008 22:38:18 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37872</guid>
		<description>Quantum mechanics is the unitary evolution of a wave function, which completely preserves quantum information (Q-bits).  Quantum fluctuations are really a manifestation of measurement, or some decherent process, when a quantum system couples to some unspecified set of states.  These states can be in a measurement apparatus.  Yet pure quantum mechanics is perfectly time reversal invariant and preserves all the information in the initial conditions of a quantum system.

Lawrence B. Crowell</description>
		<content:encoded><![CDATA[<p>Quantum mechanics is the unitary evolution of a wave function, which completely preserves quantum information (Q-bits).  Quantum fluctuations are really a manifestation of measurement, or some decherent process, when a quantum system couples to some unspecified set of states.  These states can be in a measurement apparatus.  Yet pure quantum mechanics is perfectly time reversal invariant and preserves all the information in the initial conditions of a quantum system.</p>
<p>Lawrence B. Crowell</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: John Merryman</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37862</link>
		<dc:creator>John Merryman</dc:creator>
		<pubDate>Tue, 11 Mar 2008 21:06:56 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37862</guid>
		<description>Lawrence,

Doesn&#039;t the Uncertainty Principle essentially show that some information is destroyed in the very process of measuring other information?

 Since I view time as a consequence of motion, rather than the dimensional basis for it, I think monumental amounts of information are destroyed and replaced every moment. I would posit the current credit meltdown, as well as the rest of history, as proof.</description>
		<content:encoded><![CDATA[<p>Lawrence,</p>
<p>Doesn&#8217;t the Uncertainty Principle essentially show that some information is destroyed in the very process of measuring other information?</p>
<p> Since I view time as a consequence of motion, rather than the dimensional basis for it, I think monumental amounts of information are destroyed and replaced every moment. I would posit the current credit meltdown, as well as the rest of history, as proof.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Lawrence B. Crowell</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37871</link>
		<dc:creator>Lawrence B. Crowell</dc:creator>
		<pubDate>Tue, 11 Mar 2008 19:55:51 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37871</guid>
		<description>If inflation expanded a small spherical cosmology into a flat spacetime, this spacetime may well be of infinite extent.  A finite cosmology, or a three dimensional ball with a two dimensional boundary, requires that boundary conditions exist there.  This is somewhat problematic.  However, even for an infinite dimensional R^3 space the topology change likely means that some topological information is either lost (destroyed) or is transformed into some other form.  What that is is difficult to say, maybe a &#039;t Hooft-Polyakov monopole.

Lawrence B. Crowell</description>
		<content:encoded><![CDATA[<p>If inflation expanded a small spherical cosmology into a flat spacetime, this spacetime may well be of infinite extent.  A finite cosmology, or a three dimensional ball with a two dimensional boundary, requires that boundary conditions exist there.  This is somewhat problematic.  However, even for an infinite dimensional R^3 space the topology change likely means that some topological information is either lost (destroyed) or is transformed into some other form.  What that is is difficult to say, maybe a &#8216;t Hooft-Polyakov monopole.</p>
<p>Lawrence B. Crowell</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: John Merryman</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37843</link>
		<dc:creator>John Merryman</dc:creator>
		<pubDate>Tue, 11 Mar 2008 02:28:11 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37843</guid>
		<description>Spaceman,

 According to Inflation theory, it is many, many times the size of the visible universe. To the point that, from our perspective, it is just about spatially infinite. Curvature seems mostly a function of the time dimension, in that the analysis of redshift and CMBR says it is only13.73 billion years old.

http://en.wikipedia.org/wiki/Cosmic_inflation

&quot;Cosmic inflation has the important effect of smoothing out inhomogeneities, anisotropies and the curvature of space.&quot;

 Basically it explains how the factors which suggest an infinite universe can exist in a finite model.</description>
		<content:encoded><![CDATA[<p>Spaceman,</p>
<p> According to Inflation theory, it is many, many times the size of the visible universe. To the point that, from our perspective, it is just about spatially infinite. Curvature seems mostly a function of the time dimension, in that the analysis of redshift and CMBR says it is only13.73 billion years old.</p>
<p><a href="http://en.wikipedia.org/wiki/Cosmic_inflation" rel="nofollow">http://en.wikipedia.org/wiki/Cosmic_inflation</a></p>
<p>&#8220;Cosmic inflation has the important effect of smoothing out inhomogeneities, anisotropies and the curvature of space.&#8221;</p>
<p> Basically it explains how the factors which suggest an infinite universe can exist in a finite model.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Lawrence B. Crowell</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/comment-page-1/#comment-37870</link>
		<dc:creator>Lawrence B. Crowell</dc:creator>
		<pubDate>Tue, 11 Mar 2008 00:05:26 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2008/03/05/wmap-5-year-results-released/#comment-37870</guid>
		<description>Jason Dick on Mar 10th, 2008 at 1:19 pm
Secret American Planck Basher,

Well, the free parameter in question is a pretty important one, in my view: the energy scale of inflation. Pinning down the energy scale of inflation is a pretty big step in making any significant statements about what inflation actually is.

-----------------

In cosmology the time dependency of the metric coefficients means there is no Killing vector which as an isometry defines an energy conservation.  As strange as it might sound, conservation of energy in cosmology is not definable.  The only conservation law we really have is the continuity equation

$latex
\nabla_aT^{ab}~=~0
$

plus conservation based what ever spatial killing vectors might exist.

Lawrence B. Crowell</description>
		<content:encoded><![CDATA[<p>Jason Dick on Mar 10th, 2008 at 1:19 pm<br />
Secret American Planck Basher,</p>
<p>Well, the free parameter in question is a pretty important one, in my view: the energy scale of inflation. Pinning down the energy scale of inflation is a pretty big step in making any significant statements about what inflation actually is.</p>
<p>&#8212;&#8212;&#8212;&#8212;&#8212;&#8211;</p>
<p>In cosmology the time dependency of the metric coefficients means there is no Killing vector which as an isometry defines an energy conservation.  As strange as it might sound, conservation of energy in cosmology is not definable.  The only conservation law we really have is the continuity equation</p>
<p>$latex<br />
\nabla_aT^{ab}~=~0<br />
$</p>
<p>plus conservation based what ever spatial killing vectors might exist.</p>
<p>Lawrence B. Crowell</p>
]]></content:encoded>
	</item>
</channel>
</rss>
