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	<title>Comments on: How to Go After Dark Energy?</title>
	<atom:link href="http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/</link>
	<description>Random samplings from a universe of ideas.</description>
	<lastBuildDate>Tue, 24 Nov 2009 07:08:48 -0600</lastBuildDate>
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		<title>By: shantanu</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108869</link>
		<dc:creator>shantanu</dc:creator>
		<pubDate>Sun, 01 Nov 2009 00:11:18 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108869</guid>
		<description>talking of LISA, anyone know the status of LISA path-finder? It was supposed to be launched in Oct. 2009?</description>
		<content:encoded><![CDATA[<p>talking of LISA, anyone know the status of LISA path-finder? It was supposed to be launched in Oct. 2009?</p>
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		<title>By: likaifang</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108820</link>
		<dc:creator>likaifang</dc:creator>
		<pubDate>Fri, 30 Oct 2009 05:55:53 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108820</guid>
		<description>Oh,That&#039;s bad news,I think it is a mission worth to do.</description>
		<content:encoded><![CDATA[<p>Oh,That&#8217;s bad news,I think it is a mission worth to do.</p>
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		<title>By: Eugene</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108782</link>
		<dc:creator>Eugene</dc:creator>
		<pubDate>Thu, 29 Oct 2009 18:19:18 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108782</guid>
		<description>Doug,

I understand the arguments pro/con of BEPAC. I am not saying I disagree with BEPAC&#039;s choice, I am just calling out Tod&#039;s statement that JDEM is a small portion of the pie, which is of course, not true.

Eugene</description>
		<content:encoded><![CDATA[<p>Doug,</p>
<p>I understand the arguments pro/con of BEPAC. I am not saying I disagree with BEPAC&#8217;s choice, I am just calling out Tod&#8217;s statement that JDEM is a small portion of the pie, which is of course, not true.</p>
<p>Eugene</p>
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		<title>By: Sili</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108768</link>
		<dc:creator>Sili</dc:creator>
		<pubDate>Thu, 29 Oct 2009 11:07:43 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108768</guid>
		<description>Is there more to this mission than &#039;just&#039; very accurate measurements of SN1As? If not, why is a dedicated probe necessary - it would seem to be a job a more &#039;all-round&#039; telescope could do. I&#039;m not saying we need a new Hubble (but we need a new Hubble), but a satellite that could do two or three things at once might do the trick.

How thick on the ground are super novae? Would it be possible to use the space telescope in question to do one kind of &#039;boring&#039; observation most of the time, and then just turn it around whenever the fireworks go off?

Of course, I&#039;m ignorant and have my biases - I&#039;m not really fond of Kepler, even if it does what it does very well. To be fair I probably should look up how much that cost. (And I&#039;m being unfair since I lurrrrrrve the dedicated missions of WMAP and Planck.)</description>
		<content:encoded><![CDATA[<p>Is there more to this mission than &#8216;just&#8217; very accurate measurements of SN1As? If not, why is a dedicated probe necessary &#8211; it would seem to be a job a more &#8216;all-round&#8217; telescope could do. I&#8217;m not saying we need a new Hubble (but we need a new Hubble), but a satellite that could do two or three things at once might do the trick.</p>
<p>How thick on the ground are super novae? Would it be possible to use the space telescope in question to do one kind of &#8216;boring&#8217; observation most of the time, and then just turn it around whenever the fireworks go off?</p>
<p>Of course, I&#8217;m ignorant and have my biases &#8211; I&#8217;m not really fond of Kepler, even if it does what it does very well. To be fair I probably should look up how much that cost. (And I&#8217;m being unfair since I lurrrrrrve the dedicated missions of WMAP and Planck.)</p>
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		<title>By: Timon of Athens</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108762</link>
		<dc:creator>Timon of Athens</dc:creator>
		<pubDate>Thu, 29 Oct 2009 05:19:23 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108762</guid>
		<description>&quot;, if the dark energy were not simply vacuum energy; but right now we have no compelling reason to think it’s not&quot;

Actually, we have no compelling reason to believe either way: see for example

http://arxiv.org/abs/0910.0252

There are degeneracies all over the place, and breaking them is all-important.</description>
		<content:encoded><![CDATA[<p>&#8220;, if the dark energy were not simply vacuum energy; but right now we have no compelling reason to think it’s not&#8221;</p>
<p>Actually, we have no compelling reason to believe either way: see for example</p>
<p><a href="http://arxiv.org/abs/0910.0252" rel="nofollow">http://arxiv.org/abs/0910.0252</a></p>
<p>There are degeneracies all over the place, and breaking them is all-important.</p>
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		<title>By: Brian Gerke</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108748</link>
		<dc:creator>Brian Gerke</dc:creator>
		<pubDate>Thu, 29 Oct 2009 03:00:33 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108748</guid>
		<description>Doug,

Thanks for making my oblique implications more explicit. :)

I can&#039;t imagine how any space-based mission would be worth the cost without enabling lots of ancillary science besides DE.  Thousands of square degrees of Hubble-like imaging?  Yes, please.</description>
		<content:encoded><![CDATA[<p>Doug,</p>
<p>Thanks for making my oblique implications more explicit. <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
<p>I can&#8217;t imagine how any space-based mission would be worth the cost without enabling lots of ancillary science besides DE.  Thousands of square degrees of Hubble-like imaging?  Yes, please.</p>
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		<title>By: Doug</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108738</link>
		<dc:creator>Doug</dc:creator>
		<pubDate>Thu, 29 Oct 2009 01:12:51 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108738</guid>
		<description>I should also add, if you use weak lensing as one of the probes of DE in JDEM, you get several thousand square degrees of space quality imaging along with redshift information for all of the galaxies in that area (photo-z&#039;s at least).  Even if you don&#039;t think DE is worth studying, the amount of additional science which such a dataset would produce would be immense, and probably worth the cost of the mission by itself.</description>
		<content:encoded><![CDATA[<p>I should also add, if you use weak lensing as one of the probes of DE in JDEM, you get several thousand square degrees of space quality imaging along with redshift information for all of the galaxies in that area (photo-z&#8217;s at least).  Even if you don&#8217;t think DE is worth studying, the amount of additional science which such a dataset would produce would be immense, and probably worth the cost of the mission by itself.</p>
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		<title>By: Doug</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108737</link>
		<dc:creator>Doug</dc:creator>
		<pubDate>Thu, 29 Oct 2009 01:06:37 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108737</guid>
		<description>Eugene,

JDEM emerged from BEPAC because  LISA et al were untested (and in many cases yet to be developed) technologies which would cost well in excess of JDEM.  As BEPAC was tasked with deciding which of the Beyond Einstein probes should be the first to be built in a budget situation where you could only build one in the next x years (I think 5, I forget the actual number), they concluded (wisely imo) that the one that uses known technology is probably the best bet.  

Any multi-satellite mission is unproven technology, so would likely require a pre-LISA mission to develop that technology before starting the LISA design.  If JDEM were to be funded, you&#039;d be draining a portion of LISA&#039;s development budget, nowhere close to the full budget.  Really the only argument worth having (among the BE designs) for a near term mission is a JDEM vs a descoped SIM vs a descoped con-X (or whatever the current name for it is, as it can&#039;t be a multi-satellite constellation mission).</description>
		<content:encoded><![CDATA[<p>Eugene,</p>
<p>JDEM emerged from BEPAC because  LISA et al were untested (and in many cases yet to be developed) technologies which would cost well in excess of JDEM.  As BEPAC was tasked with deciding which of the Beyond Einstein probes should be the first to be built in a budget situation where you could only build one in the next x years (I think 5, I forget the actual number), they concluded (wisely imo) that the one that uses known technology is probably the best bet.  </p>
<p>Any multi-satellite mission is unproven technology, so would likely require a pre-LISA mission to develop that technology before starting the LISA design.  If JDEM were to be funded, you&#8217;d be draining a portion of LISA&#8217;s development budget, nowhere close to the full budget.  Really the only argument worth having (among the BE designs) for a near term mission is a JDEM vs a descoped SIM vs a descoped con-X (or whatever the current name for it is, as it can&#8217;t be a multi-satellite constellation mission).</p>
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		<title>By: Brian Gerke</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108736</link>
		<dc:creator>Brian Gerke</dc:creator>
		<pubDate>Thu, 29 Oct 2009 00:30:50 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108736</guid>
		<description>The implication here that BigBOSS is the DOE&#039;s threat to give up on a satellite altogether strikes me as a misunderstanding.  

As I understand it, BigBOSS is a smallish team of scientists, not all from DOE, claiming that a particular observational strategy for JDEM (acoustic oscillations with photometry, and nothing else), which had been gaining traction, can be done around 10x more cheaply from the ground than from space.  To drive home the point, they then proposed to do the ground-based survey.  

But this isn&#039;t the same as DOE &quot;giving up&quot; on a satellite, it&#039;s just some scientists arguing, correctly, that the science needs to justify the cost: if you&#039;re going to to to space, the science return had better be waaay better than what you can get from the ground.  If the BigBOSS claims are correct (and I&#039;m not in a position to say), then JDEM will only be worth it with a more comprehensive approach in terms of the number of DE probes it considers.  (The fact that DOE folks had such a strategy in mind is possibly relevant here, though.)</description>
		<content:encoded><![CDATA[<p>The implication here that BigBOSS is the DOE&#8217;s threat to give up on a satellite altogether strikes me as a misunderstanding.  </p>
<p>As I understand it, BigBOSS is a smallish team of scientists, not all from DOE, claiming that a particular observational strategy for JDEM (acoustic oscillations with photometry, and nothing else), which had been gaining traction, can be done around 10x more cheaply from the ground than from space.  To drive home the point, they then proposed to do the ground-based survey.  </p>
<p>But this isn&#8217;t the same as DOE &#8220;giving up&#8221; on a satellite, it&#8217;s just some scientists arguing, correctly, that the science needs to justify the cost: if you&#8217;re going to to to space, the science return had better be waaay better than what you can get from the ground.  If the BigBOSS claims are correct (and I&#8217;m not in a position to say), then JDEM will only be worth it with a more comprehensive approach in terms of the number of DE probes it considers.  (The fact that DOE folks had such a strategy in mind is possibly relevant here, though.)</p>
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		<title>By: Chris Hirata</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2009/10/28/how-to-go-after-dark-energy/comment-page-1/#comment-108734</link>
		<dc:creator>Chris Hirata</dc:creator>
		<pubDate>Wed, 28 Oct 2009 22:30:01 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=3090#comment-108734</guid>
		<description>Sean,

First, there&#039;s an underlying difference of philosophy here of what to do given that one model for DE (Lambda) stands out as the &quot;simplest&quot;.  Some people would argue that this means it should be de-prioritized because the &quot;probability&quot; of alternatives to Lambda is small.  An alternative viewpoint is that having one theoretically favored model that makes a definite prediction (i.e. where the theory says you shouldn&#039;t need additional fudge parameters) warrants increased priority.

I also think we may have different notions of what &quot;nearly constant in time&quot; means.  Exactly constant in time means rho[DE]~a^0 (where a is scale factor).  A 0.07 (1 sigma) error in w means that we know the exponent of a to an uncertainty of 0.2 (1 sigma) or 0.4 (2 sigma).  The Nature article repeats the common oversimplification (sometimes made by me too!) that this means DE &quot;is constant with a precision of 7%&quot;.  Well, not quite.  In particular, I disagree with the notion that Lambda is already well enough tested to &quot;check the box&quot;.

As for how we go after DE: if you really do want an ulcer, &quot;my cosmological probe is better than your cosmological probe&quot; is a great argument to have :)

Cheers,
Chris</description>
		<content:encoded><![CDATA[<p>Sean,</p>
<p>First, there&#8217;s an underlying difference of philosophy here of what to do given that one model for DE (Lambda) stands out as the &#8220;simplest&#8221;.  Some people would argue that this means it should be de-prioritized because the &#8220;probability&#8221; of alternatives to Lambda is small.  An alternative viewpoint is that having one theoretically favored model that makes a definite prediction (i.e. where the theory says you shouldn&#8217;t need additional fudge parameters) warrants increased priority.</p>
<p>I also think we may have different notions of what &#8220;nearly constant in time&#8221; means.  Exactly constant in time means rho[DE]~a^0 (where a is scale factor).  A 0.07 (1 sigma) error in w means that we know the exponent of a to an uncertainty of 0.2 (1 sigma) or 0.4 (2 sigma).  The Nature article repeats the common oversimplification (sometimes made by me too!) that this means DE &#8220;is constant with a precision of 7%&#8221;.  Well, not quite.  In particular, I disagree with the notion that Lambda is already well enough tested to &#8220;check the box&#8221;.</p>
<p>As for how we go after DE: if you really do want an ulcer, &#8220;my cosmological probe is better than your cosmological probe&#8221; is a great argument to have <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
<p>Cheers,<br />
Chris</p>
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