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	<title>Comments on: Cosmic Variance on bloggingheads.tv</title>
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	<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/</link>
	<description>Random samplings from a universe of ideas.</description>
	<lastBuildDate>Sun, 08 Nov 2009 06:06:50 -0600</lastBuildDate>
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		<item>
		<title>By: Shantanu</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-80607</link>
		<dc:creator>Shantanu</dc:creator>
		<pubDate>Sun, 28 Jun 2009 18:24:04 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-80607</guid>
		<description>Sean, I think I may have asked you this. But do you think that Milgrom&#039;s relations could be telling
us something about the nature of the dark matter (rather than modified gravity) and that it cannot be a
a vanilla WIMP, but has to be more exotic.? AFAIk, 
the only person who has advocated this pov is Luc Blanchet  who argued that dark matter consists of dipolar medium.  Or does the bullet cluster rule out his proposed dark matter model?
Nevertheless from listening to this conversation, it seems  you agree that Milgrom&#039;s relations are a fact and have to be explained, right?
Thanks</description>
		<content:encoded><![CDATA[<p>Sean, I think I may have asked you this. But do you think that Milgrom&#8217;s relations could be telling<br />
us something about the nature of the dark matter (rather than modified gravity) and that it cannot be a<br />
a vanilla WIMP, but has to be more exotic.? AFAIk,<br />
the only person who has advocated this pov is Luc Blanchet  who argued that dark matter consists of dipolar medium.  Or does the bullet cluster rule out his proposed dark matter model?<br />
Nevertheless from listening to this conversation, it seems  you agree that Milgrom&#8217;s relations are a fact and have to be explained, right?<br />
Thanks</p>
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	<item>
		<title>By: Dave</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-80470</link>
		<dc:creator>Dave</dc:creator>
		<pubDate>Sat, 27 Jun 2009 11:52:45 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-80470</guid>
		<description>I don&#039;t usually have the chance to listen to two astrophysicists describing the universe. Sometimes the internets are great.</description>
		<content:encoded><![CDATA[<p>I don&#8217;t usually have the chance to listen to two astrophysicists describing the universe. Sometimes the internets are great.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Brendan</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79807</link>
		<dc:creator>Brendan</dc:creator>
		<pubDate>Mon, 22 Jun 2009 07:51:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79807</guid>
		<description>@Steve:

If you visit the &lt;a href=&quot;http://bloggingheads.tv/diavlogs/20597&quot; rel=&quot;nofollow&quot;&gt;diavlog page&lt;/a&gt;, you can find a link to the MP3 file containing the audio-only portion of the diavlog, right below the video window and list of topics.  (You can also download video files (WMV or MP4), for anyone else who might be interested.)</description>
		<content:encoded><![CDATA[<p>@Steve:</p>
<p>If you visit the <a href="http://bloggingheads.tv/diavlogs/20597" rel="nofollow">diavlog page</a>, you can find a link to the MP3 file containing the audio-only portion of the diavlog, right below the video window and list of topics.  (You can also download video files (WMV or MP4), for anyone else who might be interested.)</p>
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	<item>
		<title>By: Steve</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79800</link>
		<dc:creator>Steve</dc:creator>
		<pubDate>Mon, 22 Jun 2009 04:49:02 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79800</guid>
		<description>Since it&#039;s just talking heads, it would be nice to have an mp3 file of the audio to listen to while away from the computer.</description>
		<content:encoded><![CDATA[<p>Since it&#8217;s just talking heads, it would be nice to have an mp3 file of the audio to listen to while away from the computer.</p>
]]></content:encoded>
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	<item>
		<title>By: Sean</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79786</link>
		<dc:creator>Sean</dc:creator>
		<pubDate>Mon, 22 Jun 2009 00:32:47 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79786</guid>
		<description>Starwatcher--  If you believe we live in a special place in the universe, very strange distance/redshift relations are possible.  There are some constraints, but as I recall (I may be out of date) they&#039;re not very good.

Objects sufficiently far away are always moving faster than the speed of light, if the expanding universe is big enough.  Dark energy is responsible for accelerated expansion: the apparent velocity of individual galaxies is increasing with time.  &quot;Inflation&quot; refers specifically to accelerated expansion in the early universe.

Yes, we think that a&#039; and a&quot; are both positive right now.  That&#039;s from real measurements.  The Hubble parameter is a&#039;/a, which is actually decreasing. although slowly.

Zero point energy is one possible example of dark energy.  It produces effects through its influence on gravity (spacetime curvature).  &quot;Only differences in energy are observable&quot; is not true once you include gravity.

It&#039;s hard to measure velocities without using redshifts.  You might look at Ned Wright&#039;s tutorial for more info:

http://www.astro.ucla.edu/~wright/cosmolog.htm</description>
		<content:encoded><![CDATA[<p>Starwatcher&#8211;  If you believe we live in a special place in the universe, very strange distance/redshift relations are possible.  There are some constraints, but as I recall (I may be out of date) they&#8217;re not very good.</p>
<p>Objects sufficiently far away are always moving faster than the speed of light, if the expanding universe is big enough.  Dark energy is responsible for accelerated expansion: the apparent velocity of individual galaxies is increasing with time.  &#8220;Inflation&#8221; refers specifically to accelerated expansion in the early universe.</p>
<p>Yes, we think that a&#8217; and a&#8221; are both positive right now.  That&#8217;s from real measurements.  The Hubble parameter is a&#8217;/a, which is actually decreasing. although slowly.</p>
<p>Zero point energy is one possible example of dark energy.  It produces effects through its influence on gravity (spacetime curvature).  &#8220;Only differences in energy are observable&#8221; is not true once you include gravity.</p>
<p>It&#8217;s hard to measure velocities without using redshifts.  You might look at Ned Wright&#8217;s tutorial for more info:</p>
<p><a href="http://www.astro.ucla.edu/~wright/cosmolog.htm" rel="nofollow">http://www.astro.ucla.edu/~wright/cosmolog.htm</a></p>
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	<item>
		<title>By: Starwatcher162536</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79781</link>
		<dc:creator>Starwatcher162536</dc:creator>
		<pubDate>Sun, 21 Jun 2009 22:30:05 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79781</guid>
		<description>Hi, here are a few questions I had after watching you two on Bloggingheads.

[B](.5A)[/B]Is there anyway to prove that we are not in the center of the universe with a linear redshift-distance law as opposed to being in the center with a quadratic redshift-distance law?

[B](A)[/B]I was under the impression, that since anything outside the Hubble radius is receding at values above c{z&gt;C}, current theory is that the universe is still inflating, albeit much much slower then right after the Big Bang. Is dark energy what is suppose to be driving this inflation?

[B](B)[/B]If the above is true, then that means that a&#039;(t) and a&quot;(t) are &gt;0, has this been measured? Is this why Hubble&#039;s constant is said to be decreasing? But doesn&#039;t this contradict the inflation model, since if a&#039;(t) is increasing exponentially (like I would expect if the expansion depends on the volume of the universe) the constant should have a steady value, whats going on?

[B](B.5)[/B]Is there any difference between dark energy and zero point energy? If not, how can dark energy actually produce any effects? I thought the only reason you could subtract out the infinities of ground states is because only differences in energy are measurable. But since it is producing changes, does this mean the zero point energy is interacting with something outside our universe that has a even lower ground state?

[B](C)[/B]Since the Freidman equations depend on a isotropic universe (k can only have discrete values), what methods do we have to measure the receding velocities of distant objects that do not depend on the redshift?</description>
		<content:encoded><![CDATA[<p>Hi, here are a few questions I had after watching you two on Bloggingheads.</p>
<p>[B](.5A)[/B]Is there anyway to prove that we are not in the center of the universe with a linear redshift-distance law as opposed to being in the center with a quadratic redshift-distance law?</p>
<p>[B](A)[/B]I was under the impression, that since anything outside the Hubble radius is receding at values above c{z>C}, current theory is that the universe is still inflating, albeit much much slower then right after the Big Bang. Is dark energy what is suppose to be driving this inflation?</p>
<p>[B](B)[/B]If the above is true, then that means that a&#8217;(t) and a&#8221;(t) are >0, has this been measured? Is this why Hubble&#8217;s constant is said to be decreasing? But doesn&#8217;t this contradict the inflation model, since if a&#8217;(t) is increasing exponentially (like I would expect if the expansion depends on the volume of the universe) the constant should have a steady value, whats going on?</p>
<p>[B](B.5)[/B]Is there any difference between dark energy and zero point energy? If not, how can dark energy actually produce any effects? I thought the only reason you could subtract out the infinities of ground states is because only differences in energy are measurable. But since it is producing changes, does this mean the zero point energy is interacting with something outside our universe that has a even lower ground state?</p>
<p>[B](C)[/B]Since the Freidman equations depend on a isotropic universe (k can only have discrete values), what methods do we have to measure the receding velocities of distant objects that do not depend on the redshift?</p>
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	<item>
		<title>By: Peter Coles</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79774</link>
		<dc:creator>Peter Coles</dc:creator>
		<pubDate>Sun, 21 Jun 2009 21:03:16 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79774</guid>
		<description>For some reason this reminded me of Thunderbirds.
FAB!</description>
		<content:encoded><![CDATA[<p>For some reason this reminded me of Thunderbirds.<br />
FAB!</p>
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		<title>By: The Science Pundit</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79765</link>
		<dc:creator>The Science Pundit</dc:creator>
		<pubDate>Sun, 21 Jun 2009 19:15:55 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79765</guid>
		<description>I really enjoyed that.  Unfortunately, I&#039;m just as confused about the deeper cosmological questions now as I was before watching.  Maybe one of these days it will all start to make sense.  :-/</description>
		<content:encoded><![CDATA[<p>I really enjoyed that.  Unfortunately, I&#8217;m just as confused about the deeper cosmological questions now as I was before watching.  Maybe one of these days it will all start to make sense.  :-/</p>
]]></content:encoded>
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		<title>By: Brendan</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79720</link>
		<dc:creator>Brendan</dc:creator>
		<pubDate>Sun, 21 Jun 2009 06:03:50 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79720</guid>
		<description>I did enjoy this diavlog, very much, and I hope you and Sean do at least one more of these soon.</description>
		<content:encoded><![CDATA[<p>I did enjoy this diavlog, very much, and I hope you and Sean do at least one more of these soon.</p>
]]></content:encoded>
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		<title>By: ZachB</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/comment-page-1/#comment-79719</link>
		<dc:creator>ZachB</dc:creator>
		<pubDate>Sun, 21 Jun 2009 05:31:29 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2009/06/20/cosmic-variance-on-bloggingheadstv/#comment-79719</guid>
		<description>Haha, seesaw mechanism.</description>
		<content:encoded><![CDATA[<p>Haha, seesaw mechanism.</p>
]]></content:encoded>
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