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	<title>Comments on: Return to the Fold</title>
	<atom:link href="http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/</link>
	<description>Random samplings from a universe of ideas.</description>
	<lastBuildDate>Tue, 14 Feb 2012 14:15:44 +0000</lastBuildDate>
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	<item>
		<title>By: PLato</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-11003</link>
		<dc:creator>PLato</dc:creator>
		<pubDate>Mon, 30 Jan 2006 17:56:12 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-11003</guid>
		<description>Layman scratching

amazing...that viscosity measures(D brane analysis?) could have been hidden in all this talk?</description>
		<content:encoded><![CDATA[<p>Layman scratching</p>
<p>amazing&#8230;that viscosity measures(D brane analysis?) could have been hidden in all this talk?</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Nick Evans</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-11002</link>
		<dc:creator>Nick Evans</dc:creator>
		<pubDate>Mon, 30 Jan 2006 17:21:06 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-11002</guid>
		<description>Hi Guys. Thanks for your interest in our paper on ghost branes and SU(N&#124;N) regularization.

I&#039;ll let Olly try to convince you about regulators - as you&#039;ve deduced it&#039;s basically the same story as Pauli Villars though.

Flat space as a dual I can try to be helpful for you though. Stay in the pure AdS/CFT Correspondence - move the D3 onto a 5-sphere. The geometry is AdS outside the sphere and flat space inside. What does that mean? It means the theory is totally higgsed at the scale corresponding to the radius of the sphere and below that scale is a mass gap. The gravity description of this &quot;nothing&quot; is flat space. Our host, Clifford, played precisely this game in his enhancon papers removing repulsons and replacing with flat space...

cheers Nick</description>
		<content:encoded><![CDATA[<p>Hi Guys. Thanks for your interest in our paper on ghost branes and SU(N|N) regularization.</p>
<p>I&#8217;ll let Olly try to convince you about regulators &#8211; as you&#8217;ve deduced it&#8217;s basically the same story as Pauli Villars though.</p>
<p>Flat space as a dual I can try to be helpful for you though. Stay in the pure AdS/CFT Correspondence &#8211; move the D3 onto a 5-sphere. The geometry is AdS outside the sphere and flat space inside. What does that mean? It means the theory is totally higgsed at the scale corresponding to the radius of the sphere and below that scale is a mass gap. The gravity description of this &#8220;nothing&#8221; is flat space. Our host, Clifford, played precisely this game in his enhancon papers removing repulsons and replacing with flat space&#8230;</p>
<p>cheers Nick</p>
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	</item>
	<item>
		<title>By: Oliver</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-11001</link>
		<dc:creator>Oliver</dc:creator>
		<pubDate>Mon, 30 Jan 2006 16:10:38 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-11001</guid>
		<description>Hi,

I can shed some light on the issue of unitarity at finite cutoff.  As effectively said already, if the cutoff is sent to infinity, all fields in the spontaneously broken SU(N&#124;N) theory become infintely massive, with the exception of the physical SU(N) field (and an unphysical copy which is decoupled).  One of the crucial ingredients of our ERG approach - which is built in from the start - is that the partition function is invariant under the flow. Since we know that we are dealing with just SU(N) YM at the top end of the flow, we know that we must be dealing with the same theory everywhere along the flow. So, when computing physical quantities, the unphysical fields serve only to regularize the physical theory, and do not spoil unitarity. This works at finite N.

Oliver.</description>
		<content:encoded><![CDATA[<p>Hi,</p>
<p>I can shed some light on the issue of unitarity at finite cutoff.  As effectively said already, if the cutoff is sent to infinity, all fields in the spontaneously broken SU(N|N) theory become infintely massive, with the exception of the physical SU(N) field (and an unphysical copy which is decoupled).  One of the crucial ingredients of our ERG approach &#8211; which is built in from the start &#8211; is that the partition function is invariant under the flow. Since we know that we are dealing with just SU(N) YM at the top end of the flow, we know that we must be dealing with the same theory everywhere along the flow. So, when computing physical quantities, the unphysical fields serve only to regularize the physical theory, and do not spoil unitarity. This works at finite N.</p>
<p>Oliver.</p>
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	</item>
	<item>
		<title>By: Jacques Distler</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-11000</link>
		<dc:creator>Jacques Distler</dc:creator>
		<pubDate>Mon, 30 Jan 2006 14:15:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-11000</guid>
		<description>Multiply by whatever factor you want, and you can get whatever nonsense you desire.

The normalization of the boundary state is fixed by demanding that the open string partition function is properly normalized in the presence of boundaries.

Perhaps it might be helpful to note that one can, technically, put either bosonic or fermionic Chan-Paton factors on the boundary; you get the same answer either way. Usually, this is thought of as an either/or  proposition. The ghost D-brane proposal is to allow &lt;em&gt;both&lt;/em&gt; bosonic and fermionic Chan-Paton factors in the same theory.</description>
		<content:encoded><![CDATA[<p>Multiply by whatever factor you want, and you can get whatever nonsense you desire.</p>
<p>The normalization of the boundary state is fixed by demanding that the open string partition function is properly normalized in the presence of boundaries.</p>
<p>Perhaps it might be helpful to note that one can, technically, put either bosonic or fermionic Chan-Paton factors on the boundary; you get the same answer either way. Usually, this is thought of as an either/or  proposition. The ghost D-brane proposal is to allow <em>both</em> bosonic and fermionic Chan-Paton factors in the same theory.</p>
]]></content:encoded>
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		<title>By: Robert</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10999</link>
		<dc:creator>Robert</dc:creator>
		<pubDate>Mon, 30 Jan 2006 14:07:03 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10999</guid>
		<description>So, if I multiply by a phase do I really get branes with complex tension?</description>
		<content:encoded><![CDATA[<p>So, if I multiply by a phase do I really get branes with complex tension?</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Jacques Distler</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10998</link>
		<dc:creator>Jacques Distler</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:58:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10998</guid>
		<description>&lt;blockquote&gt;Shouldn&#039;t I normalize this somehow with &lt;B&#124;B&#039;&gt;&lt;/blockquote&gt;

No! Because &lt;B&#124;B&#039;&gt;=&#8734; !

The Boundary State is not a normalizable state in the Hilbert space.</description>
		<content:encoded><![CDATA[<blockquote><p>Shouldn&#8217;t I normalize this somehow with &lt;B|B&#8217;&gt;</p></blockquote>
<p>No! Because &lt;B|B&#8217;&gt;=&infin; !</p>
<p>The Boundary State is not a normalizable state in the Hilbert space.</p>
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	</item>
	<item>
		<title>By: Robert</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10997</link>
		<dc:creator>Robert</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:42:59 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10997</guid>
		<description>&lt;/em&gt;
I could ask the same question in ordinary QFT: I can &#039;probe&#039; the charge of a particle by computing the amplitude for a T-channel exchange of a photon. That should be proportional to e^2. However, I do not get ghost electrons with positive charge and negative mass by multiplying external electron lines by (-1).</description>
		<content:encoded><![CDATA[<p>I could ask the same question in ordinary QFT: I can &#8216;probe&#8217; the charge of a particle by computing the amplitude for a T-channel exchange of a photon. That should be proportional to e^2. However, I do not get ghost electrons with positive charge and negative mass by multiplying external electron lines by (-1).</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Robert</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10996</link>
		<dc:creator>Robert</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:38:39 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10996</guid>
		<description>? was langle B&#124;B rangle</description>
		<content:encoded><![CDATA[<p>? was langle B|B rangle</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Robert</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10995</link>
		<dc:creator>Robert</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:38:18 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10995</guid>
		<description>Shouldn&#039;t I normalize this somehow with &lt; B &gt;?</description>
		<content:encoded><![CDATA[<p>Shouldn&#8217;t I normalize this somehow with < B >?</p>
]]></content:encoded>
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		<title>By: Jacques Distler</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10994</link>
		<dc:creator>Jacques Distler</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:16:57 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10994</guid>
		<description>Whoa! Cool! I can mess up, not only my own comment, but succeeding ones as well. WordPress is &lt;em&gt;da Bomb!&lt;/em&gt;</description>
		<content:encoded><![CDATA[<p>Whoa! Cool! I can mess up, not only my own comment, but succeeding ones as well. WordPress is <em>da Bomb!</em></p>
]]></content:encoded>
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		<title>By: Jacques Distler</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10993</link>
		<dc:creator>Jacques Distler</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:15:14 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10993</guid>
		<description>Hmmm. That was amusing. Let&#039;s try that equation again, shall we?

&lt;B&#124;q^{H}&#124;B&#039;&gt;</description>
		<content:encoded><![CDATA[<p>Hmmm. That was amusing. Let&#8217;s try that equation again, shall we?</p>
<p>&lt;B|q^{H}|B&#8217;&gt;</p>
]]></content:encoded>
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		<title>By: Jacques Distler</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10992</link>
		<dc:creator>Jacques Distler</dc:creator>
		<pubDate>Mon, 30 Jan 2006 13:13:39 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10992</guid>
		<description>The open-string partition function can be written, in the closed-string channel, as
Z=.  Adding Chan-Paton factors, formally multiplies Z by a factor of N N&#039;.

So, indeed, the normalization of the boundary state matters. That&#039;s part of the data that goes into normalizing the path integral in the presence of boundaries.</description>
		<content:encoded><![CDATA[<p>The open-string partition function can be written, in the closed-string channel, as<br />
Z=.  Adding Chan-Paton factors, formally multiplies Z by a factor of N N&#8217;.</p>
<p>So, indeed, the normalization of the boundary state matters. That&#8217;s part of the data that goes into normalizing the path integral in the presence of boundaries.</p>
]]></content:encoded>
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	<item>
		<title>By: Robert</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10991</link>
		<dc:creator>Robert</dc:creator>
		<pubDate>Mon, 30 Jan 2006 11:16:03 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10991</guid>
		<description>I think I have another problem with the ghost branes. So I sent an email to the authors saying

I am surprised that by multiplying a boundary state &#124;D&gt; by (-1) you get a different state.
As you claim, a D-brane is turned into a ghost brane with opposite charges and tension.
I am a bit surprised by this since I would have thought that strictly speaking a state is not
given by a vector in a Hilbert space but by a ray in such a space. That is, only by a vector
up to normalisation by a non-zero complex number.

This would also follow from boundary CFT where the boundary state is defined by the condition
that certain operators (for example T, the left handed energy momentum tensor and its
right handed counterpart T-bar) agree on the boundary:

T&#124;boundary&gt;= T-bar&#124;boundary&gt;

But such equation again would characterise &#124;boundary&gt; at best up to a scalar multiple. So
I am quite surprised that a factor of (-1) has such drastic consequences. Maybe you
could comment on this?

Once we start transforming states by multiplication by (-1), nothing stops us from
considering exp(i phi)&#124;D&gt; for some phase exp(i phi). By a similar argument as yours,
I would conclude that this rotated state has a complex mass and charge since the
phase also multiplies amplitudes like



Is that correct?


I got a reply which I am not sure I am supposed to quote. It said something along the lines of the boundary state being a classical object from the target space perspective and thus a prefactor would matter. For example by multiplying by N I would get a state of N coincident branes.

I must say this does not really convince me. Could anybody else please say something about this?</description>
		<content:encoded><![CDATA[<p>I think I have another problem with the ghost branes. So I sent an email to the authors saying</p>
<p>I am surprised that by multiplying a boundary state |D&gt; by (-1) you get a different state.<br />
As you claim, a D-brane is turned into a ghost brane with opposite charges and tension.<br />
I am a bit surprised by this since I would have thought that strictly speaking a state is not<br />
given by a vector in a Hilbert space but by a ray in such a space. That is, only by a vector<br />
up to normalisation by a non-zero complex number.</p>
<p>This would also follow from boundary CFT where the boundary state is defined by the condition<br />
that certain operators (for example T, the left handed energy momentum tensor and its<br />
right handed counterpart T-bar) agree on the boundary:</p>
<p>T|boundary&gt;= T-bar|boundary&gt;</p>
<p>But such equation again would characterise |boundary&gt; at best up to a scalar multiple. So<br />
I am quite surprised that a factor of (-1) has such drastic consequences. Maybe you<br />
could comment on this?</p>
<p>Once we start transforming states by multiplication by (-1), nothing stops us from<br />
considering exp(i phi)|D&gt; for some phase exp(i phi). By a similar argument as yours,<br />
I would conclude that this rotated state has a complex mass and charge since the<br />
phase also multiplies amplitudes like</p>
<p>Is that correct?</p>
<p>I got a reply which I am not sure I am supposed to quote. It said something along the lines of the boundary state being a classical object from the target space perspective and thus a prefactor would matter. For example by multiplying by N I would get a state of N coincident branes.</p>
<p>I must say this does not really convince me. Could anybody else please say something about this?</p>
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	<item>
		<title>By: boreds</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10990</link>
		<dc:creator>boreds</dc:creator>
		<pubDate>Sun, 29 Jan 2006 17:18:02 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10990</guid>
		<description>another thing that puzzles me is that the flat space isometries won&#039;t match up with the conformal group etc anymore</description>
		<content:encoded><![CDATA[<p>another thing that puzzles me is that the flat space isometries won&#8217;t match up with the conformal group etc anymore</p>
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		<title>By: boreds</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10989</link>
		<dc:creator>boreds</dc:creator>
		<pubDate>Sun, 29 Jan 2006 17:08:37 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10989</guid>
		<description>I agree with what you have both said, particularly that the nh limit isn&#039;t meaningful in the case n=m.

But isn&#039;t SU(n-m) when (n-m) is small dual to AdS_5xS^5 with small AdS length? If I am not missing something obvious then the same should go for SU(n&#124;m) when n-m is small.

I agree the whole geometry is flat when there are equal numbers of D and ghost-branes, but don&#039;t understand why the gauge theory is `dual&#039; to this flat geometry, as stated in the paper---probably I am missing something.</description>
		<content:encoded><![CDATA[<p>I agree with what you have both said, particularly that the nh limit isn&#8217;t meaningful in the case n=m.</p>
<p>But isn&#8217;t SU(n-m) when (n-m) is small dual to AdS_5xS^5 with small AdS length? If I am not missing something obvious then the same should go for SU(n|m) when n-m is small.</p>
<p>I agree the whole geometry is flat when there are equal numbers of D and ghost-branes, but don&#8217;t understand why the gauge theory is `dual&#8217; to this flat geometry, as stated in the paper&#8212;probably I am missing something.</p>
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		<title>By: Moshe</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10988</link>
		<dc:creator>Moshe</dc:creator>
		<pubDate>Sun, 29 Jan 2006 15:22:57 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10988</guid>
		<description>I think the statement is much more simple, SU(n&#124;m) is equivalent in some sense to SU(n-m), and is reaized as the theory on appropriate numbers of D3 and ghost D3 in flat space as usual (no decoupling limits). So when n=m one is left without any D3-branes, only with flat space.  I don&#039;t think one can take any meanigful near horizon limit with this story, maybe I am wrong.</description>
		<content:encoded><![CDATA[<p>I think the statement is much more simple, SU(n|m) is equivalent in some sense to SU(n-m), and is reaized as the theory on appropriate numbers of D3 and ghost D3 in flat space as usual (no decoupling limits). So when n=m one is left without any D3-branes, only with flat space.  I don&#8217;t think one can take any meanigful near horizon limit with this story, maybe I am wrong.</p>
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		<title>By: Clifford</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10987</link>
		<dc:creator>Clifford</dc:creator>
		<pubDate>Sun, 29 Jan 2006 14:49:57 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10987</guid>
		<description>Hi,

I don&#039;t understand why it would be highly curved AdS in that limit.  The sources of curvature seem to cancel each other out exactly (at least above a certain distance scale), and so flat space is pretty much the only option, I would say.

Cheers,

-cvj</description>
		<content:encoded><![CDATA[<p>Hi,</p>
<p>I don&#8217;t understand why it would be highly curved AdS in that limit.  The sources of curvature seem to cancel each other out exactly (at least above a certain distance scale), and so flat space is pretty much the only option, I would say.</p>
<p>Cheers,</p>
<p>-cvj</p>
]]></content:encoded>
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		<title>By: boreds</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10965</link>
		<dc:creator>boreds</dc:creator>
		<pubDate>Sun, 29 Jan 2006 02:22:58 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10965</guid>
		<description>Hi

I actually don&#039;t fully understand why SU(N&#124;N) is supposed to be dual to flat space in the ERG paper. I&#039;d expect that, as N--&gt;M, the SU(N&#124;M) theory will be dual to increasingly highly-curved AdS_5xS^5. (Even if in the case N=M the near horizon limit isn&#039;t really sensible).</description>
		<content:encoded><![CDATA[<p>Hi</p>
<p>I actually don&#8217;t fully understand why SU(N|N) is supposed to be dual to flat space in the ERG paper. I&#8217;d expect that, as N&#8211;&gt;M, the SU(N|M) theory will be dual to increasingly highly-curved AdS_5xS^5. (Even if in the case N=M the near horizon limit isn&#8217;t really sensible).</p>
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		<title>By: AndrewP</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10986</link>
		<dc:creator>AndrewP</dc:creator>
		<pubDate>Sat, 28 Jan 2006 16:44:12 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10986</guid>
		<description>One must be very cautious in extrapolating current data to infinitely accelerating acceleration of the universe until the big rip is achieved. A real world example about increasing acceleration makes that clear. Imagine that you are on the far side of an asteroid that is falling toward the earth. You observe that you are accelerating away from distant astronomical bodies and toward others without apparent explanation. But since you can&#039;t see the earth (you are on the far side), you assume that you are being moved by some mysterious dark energy. The acceleration is accelerating. Eventually it reaches 9.8 m/s2. Then smack - you hit the ground and become a giant mushroom cloud.</description>
		<content:encoded><![CDATA[<p>One must be very cautious in extrapolating current data to infinitely accelerating acceleration of the universe until the big rip is achieved. A real world example about increasing acceleration makes that clear. Imagine that you are on the far side of an asteroid that is falling toward the earth. You observe that you are accelerating away from distant astronomical bodies and toward others without apparent explanation. But since you can&#8217;t see the earth (you are on the far side), you assume that you are being moved by some mysterious dark energy. The acceleration is accelerating. Eventually it reaches 9.8 m/s2. Then smack &#8211; you hit the ground and become a giant mushroom cloud.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Elliot</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/comment-page-1/#comment-10985</link>
		<dc:creator>Elliot</dc:creator>
		<pubDate>Sat, 28 Jan 2006 16:24:24 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2006/01/27/return-to-the-fold/#comment-10985</guid>
		<description>Clifford,

Thanks. The reference to the TASI lectures looks promising.

Elliot</description>
		<content:encoded><![CDATA[<p>Clifford,</p>
<p>Thanks. The reference to the TASI lectures looks promising.</p>
<p>Elliot</p>
]]></content:encoded>
	</item>
</channel>
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