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	<title>Comments on: More Hints of Dark Matter</title>
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	<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/</link>
	<description>Random samplings from a universe of ideas.</description>
	<lastBuildDate>Fri, 25 May 2012 14:35:45 +0000</lastBuildDate>
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		<title>By: The Status of Dark Matter [Starts With A Bang] &#124; Digital Brain ; Science and Technology News</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-189620</link>
		<dc:creator>The Status of Dark Matter [Starts With A Bang] &#124; Digital Brain ; Science and Technology News</dc:creator>
		<pubDate>Fri, 21 Oct 2011 20:46:40 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-189620</guid>
		<description>[...] (Image credit: G. Angloher et al., retrieved from Sean.) [...]</description>
		<content:encoded><![CDATA[<p>[...] (Image credit: G. Angloher et al., retrieved from Sean.) [...]</p>
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	<item>
		<title>By: Dunkel-Materie-Detektion im Keller: Es steht 3:2 &#8230; &#171; Skyweek Zwei Punkt Null</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-179780</link>
		<dc:creator>Dunkel-Materie-Detektion im Keller: Es steht 3:2 &#8230; &#171; Skyweek Zwei Punkt Null</dc:creator>
		<pubDate>Thu, 15 Sep 2011 15:26:24 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-179780</guid>
		<description>[...] Verständnis der Störquellen und signifikantere Signale &#8230; Paper von Angloher &amp; al. 4., Cosmic Variance 5., DLF 6., New Scientist, BBC 7., Physics World 8., KosmoLogs 9., Science News 12., Nature News [...]</description>
		<content:encoded><![CDATA[<p>[...] Verständnis der Störquellen und signifikantere Signale &#8230; Paper von Angloher &amp; al. 4., Cosmic Variance 5., DLF 6., New Scientist, BBC 7., Physics World 8., KosmoLogs 9., Science News 12., Nature News [...]</p>
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	<item>
		<title>By: Tissa Perera</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-179531</link>
		<dc:creator>Tissa Perera</dc:creator>
		<pubDate>Wed, 14 Sep 2011 14:59:22 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-179531</guid>
		<description>The GHOST PARTCLE
But Dark Matter is more illusive than Ghosts
Some people some times have seen ghosts, but not this stuff with a big qualification...”so far”.
Dark Matter is most cosmologists play putty. It can be invoked if and when necessary and molded  conveniently  to accommodate and rectify the observed seemingly abnormal behavior of real matter in order to  save Newton’s law of gravity. To explain Dark Matter, certain obvious properties are assigned.
It must be made of some kind of  particles not resembling any of the known particles, more akin to neutrinos, but unlike neutrinos,  it must have significant mass(hence gravity), must move slow(cold) and hardly interact physically with each other or with real matter(weakly interacting) except via gravity.  I do not know why they had to attribute even a weak interaction with real matter, may be they hoped to physically detect it one day like they did with neutrinos. After so many years this stuff still remains to be detected.
The problem with such tenuous matter properties is that it cannot congregate into any significant structure except by gravity, and gravity is already a very weak force. Computer simulations have produced vast web structures of this stuff where real matter is supposed to  gravitate at the web nodes. But the visible composite structures(Galaxies etc) are moving in space at tremendous speeds. I do not  see how the dark matter web nodes flow with the real matter at these speeds without separation.
Nature may not be that way, how about modifying gravity? I have a different theory of the universe in which an extra cosmic size bounded 4th spatial dimension naturally modifies Newton’s law of gravity at cosmic scales to reproduce and modify the now famous  empirical MOND theory. Dark energy becomes a natural consequence of this theory and dark matter is not necessary. This theory basically shows that the so called dark matter is a natural consequence of the bounded curvature of the 4th space where real matter by itself is the cause of so called dark matter. Only gravity can venture into the 4th dimension which I call the dark space. After all, MOND is on the right track and MOND becomes a legitimate theory under this hypothesis.</description>
		<content:encoded><![CDATA[<p>The GHOST PARTCLE<br />
But Dark Matter is more illusive than Ghosts<br />
Some people some times have seen ghosts, but not this stuff with a big qualification&#8230;”so far”.<br />
Dark Matter is most cosmologists play putty. It can be invoked if and when necessary and molded  conveniently  to accommodate and rectify the observed seemingly abnormal behavior of real matter in order to  save Newton’s law of gravity. To explain Dark Matter, certain obvious properties are assigned.<br />
It must be made of some kind of  particles not resembling any of the known particles, more akin to neutrinos, but unlike neutrinos,  it must have significant mass(hence gravity), must move slow(cold) and hardly interact physically with each other or with real matter(weakly interacting) except via gravity.  I do not know why they had to attribute even a weak interaction with real matter, may be they hoped to physically detect it one day like they did with neutrinos. After so many years this stuff still remains to be detected.<br />
The problem with such tenuous matter properties is that it cannot congregate into any significant structure except by gravity, and gravity is already a very weak force. Computer simulations have produced vast web structures of this stuff where real matter is supposed to  gravitate at the web nodes. But the visible composite structures(Galaxies etc) are moving in space at tremendous speeds. I do not  see how the dark matter web nodes flow with the real matter at these speeds without separation.<br />
Nature may not be that way, how about modifying gravity? I have a different theory of the universe in which an extra cosmic size bounded 4th spatial dimension naturally modifies Newton’s law of gravity at cosmic scales to reproduce and modify the now famous  empirical MOND theory. Dark energy becomes a natural consequence of this theory and dark matter is not necessary. This theory basically shows that the so called dark matter is a natural consequence of the bounded curvature of the 4th space where real matter by itself is the cause of so called dark matter. Only gravity can venture into the 4th dimension which I call the dark space. After all, MOND is on the right track and MOND becomes a legitimate theory under this hypothesis.</p>
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		<title>By: forester</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-178524</link>
		<dc:creator>forester</dc:creator>
		<pubDate>Sun, 11 Sep 2011 04:54:03 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-178524</guid>
		<description>If this is some non-dark matter physical process that CRESST, CoGENT, and DAMA are detecting, then why are both XENON and CDMS not seeing evidence of the same physical process? 

I suspect that there is some background affecting the CRESST etc experiments that the XENON and CDMS teams have been able to block out.  The problem with this interpretation is that CRESST, CoGENT, and DAMA teams are run by different people and use different equipment and yet they each seem to be pointing to a new particle in a mass-range that&#039;s compatible with one another. In other words, it is not like DAMA sees evidence of a particle at 300 Gev, CRESST sees evidence at 1 mg, and CoGENT at 100 Gev. They all seem to be more or less compatible with one another from a &quot;mass of particle standpoint.&quot;</description>
		<content:encoded><![CDATA[<p>If this is some non-dark matter physical process that CRESST, CoGENT, and DAMA are detecting, then why are both XENON and CDMS not seeing evidence of the same physical process? </p>
<p>I suspect that there is some background affecting the CRESST etc experiments that the XENON and CDMS teams have been able to block out.  The problem with this interpretation is that CRESST, CoGENT, and DAMA teams are run by different people and use different equipment and yet they each seem to be pointing to a new particle in a mass-range that&#8217;s compatible with one another. In other words, it is not like DAMA sees evidence of a particle at 300 Gev, CRESST sees evidence at 1 mg, and CoGENT at 100 Gev. They all seem to be more or less compatible with one another from a &#8220;mass of particle standpoint.&#8221;</p>
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		<title>By: True_Q</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-177375</link>
		<dc:creator>True_Q</dc:creator>
		<pubDate>Fri, 09 Sep 2011 05:20:13 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-177375</guid>
		<description>You&#039;re a Time Lord? The Doctor would be happy to meet You</description>
		<content:encoded><![CDATA[<p>You&#8217;re a Time Lord? The Doctor would be happy to meet You</p>
]]></content:encoded>
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		<title>By: Liten notering om det senaste mörk materia-resultatet &#124; Stjärnstoft och kugghjul</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-177366</link>
		<dc:creator>Liten notering om det senaste mörk materia-resultatet &#124; Stjärnstoft och kugghjul</dc:creator>
		<pubDate>Fri, 09 Sep 2011 04:38:05 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-177366</guid>
		<description>[...] som vill läsa mer redan nu kan börja till exempel med inlägget på Cosmic Variance. Like this:GillaBli först att gilla denna [...]</description>
		<content:encoded><![CDATA[<p>[...] som vill läsa mer redan nu kan börja till exempel med inlägget på Cosmic Variance. Like this:GillaBli först att gilla denna [...]</p>
]]></content:encoded>
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	<item>
		<title>By: Al</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-177326</link>
		<dc:creator>Al</dc:creator>
		<pubDate>Fri, 09 Sep 2011 02:22:27 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-177326</guid>
		<description>Xenon100 doubles down with a new preprint and new analysis (arxiv, 9/8/11).

They cast considerable doubt on any &quot;WIMP&quot; sightings.

No one really believes the CRESST-II &quot;weak signal amid substantial background noise&quot;.

Nature is not &quot;messing with us&quot;, but some very misguided theoretical physicists might be.</description>
		<content:encoded><![CDATA[<p>Xenon100 doubles down with a new preprint and new analysis (arxiv, 9/8/11).</p>
<p>They cast considerable doubt on any &#8220;WIMP&#8221; sightings.</p>
<p>No one really believes the CRESST-II &#8220;weak signal amid substantial background noise&#8221;.</p>
<p>Nature is not &#8220;messing with us&#8221;, but some very misguided theoretical physicists might be.</p>
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		<title>By: Brian137</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-177005</link>
		<dc:creator>Brian137</dc:creator>
		<pubDate>Thu, 08 Sep 2011 00:53:07 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-177005</guid>
		<description>There might be several types of DM particles.</description>
		<content:encoded><![CDATA[<p>There might be several types of DM particles.</p>
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		<title>By: Research shines more light on dark matter</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176936</link>
		<dc:creator>Research shines more light on dark matter</dc:creator>
		<pubDate>Wed, 07 Sep 2011 21:04:08 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176936</guid>
		<description>[...] the CRESST experiment suggests dark matter may actually have a lower mass than previous theories.Discover Magazine&#8217;s Sean Carroll sums up the current situation best: &#8220;either the universe is really messing with us by making [...]</description>
		<content:encoded><![CDATA[<p>[...] the CRESST experiment suggests dark matter may actually have a lower mass than previous theories.Discover Magazine&#8217;s Sean Carroll sums up the current situation best: &#8220;either the universe is really messing with us by making [...]</p>
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		<title>By: Ben</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176629</link>
		<dc:creator>Ben</dc:creator>
		<pubDate>Tue, 06 Sep 2011 19:53:39 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176629</guid>
		<description>A fable to read (or re-read) for the CRESST people: &quot;The Boy Who Cried Wolf&quot; by Aesop (620-564 BCE)</description>
		<content:encoded><![CDATA[<p>A fable to read (or re-read) for the CRESST people: &#8220;The Boy Who Cried Wolf&#8221; by Aesop (620-564 BCE)</p>
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		<title>By: gameshowhost</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176584</link>
		<dc:creator>gameshowhost</dc:creator>
		<pubDate>Tue, 06 Sep 2011 17:56:18 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176584</guid>
		<description>I hear the Tea Party is already staging a protest.</description>
		<content:encoded><![CDATA[<p>I hear the Tea Party is already staging a protest.</p>
]]></content:encoded>
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		<title>By: Greg Campbell</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176576</link>
		<dc:creator>Greg Campbell</dc:creator>
		<pubDate>Tue, 06 Sep 2011 17:19:01 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176576</guid>
		<description>If WIMP mass is 20-40 GeV/c^2, the choice collision detector for selectivity, total active mass on the cheap, and sensitivity is Juan Collar&#039;s supercritical bubble chamber (arxiv:1008.3518) loaded with CCl_3F, (bp 23.7 C, d 1.49 g/cm^3.  Boiling point increases with depth given hydrostatic pressure.  Large area somewhat shallow containers will also afford directional information vs. time of day and Earth&#039;s orbital direction.  Begin synthesis with natural gas for no C-14, half-life 5715 years.  Chlorine from salt dome NaCl for no Cl-36, half-life 3x10^5 years versus 150 million years age, 500 half-lives. 

Collision energy transfer is maximum when the two bodies have equal mass, as in Newton&#039;s cradle.  If physics knows where to look, why doesn&#039;t physics look there?</description>
		<content:encoded><![CDATA[<p>If WIMP mass is 20-40 GeV/c^2, the choice collision detector for selectivity, total active mass on the cheap, and sensitivity is Juan Collar&#8217;s supercritical bubble chamber (arxiv:1008.3518) loaded with CCl_3F, (bp 23.7 C, d 1.49 g/cm^3.  Boiling point increases with depth given hydrostatic pressure.  Large area somewhat shallow containers will also afford directional information vs. time of day and Earth&#8217;s orbital direction.  Begin synthesis with natural gas for no C-14, half-life 5715 years.  Chlorine from salt dome NaCl for no Cl-36, half-life 3&#215;10^5 years versus 150 million years age, 500 half-lives. </p>
<p>Collision energy transfer is maximum when the two bodies have equal mass, as in Newton&#8217;s cradle.  If physics knows where to look, why doesn&#8217;t physics look there?</p>
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		<title>By: Hebben ze bij CRESST-II aanwijzingen voor donkere materie gevonden?</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176527</link>
		<dc:creator>Hebben ze bij CRESST-II aanwijzingen voor donkere materie gevonden?</dc:creator>
		<pubDate>Tue, 06 Sep 2011 15:30:58 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176527</guid>
		<description>[...] DAMA-LIBRA. Zouden toch collega&#8217;s moeten zijn, nietwaar? Concullega&#8217;s wellicht?  Bron: Cosmic Variance. Noot:1 pb=10−36 cm2. [&amp;#8617]Op indirecte wijze is donkere materie al lang gedetecteerd, o.a. [...]</description>
		<content:encoded><![CDATA[<p>[...] DAMA-LIBRA. Zouden toch collega&#8217;s moeten zijn, nietwaar? Concullega&#8217;s wellicht?  Bron: Cosmic Variance. Noot:1 pb=10−36 cm2. [&amp;#8617]Op indirecte wijze is donkere materie al lang gedetecteerd, o.a. [...]</p>
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		<title>By: Marc</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176443</link>
		<dc:creator>Marc</dc:creator>
		<pubDate>Tue, 06 Sep 2011 09:55:15 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176443</guid>
		<description>So, of CRESST, DAMA, COGENT and CDMSII, we can see that at least two of them must be wrong.   DAMA and COGENT are inconsistent, CDMSII and CRESST are inconsistent.    And if XENON is right, then all four of those are wrong.    Sigh....</description>
		<content:encoded><![CDATA[<p>So, of CRESST, DAMA, COGENT and CDMSII, we can see that at least two of them must be wrong.   DAMA and COGENT are inconsistent, CDMSII and CRESST are inconsistent.    And if XENON is right, then all four of those are wrong.    Sigh&#8230;.</p>
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		<title>By: Lab Lemming</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176439</link>
		<dc:creator>Lab Lemming</dc:creator>
		<pubDate>Tue, 06 Sep 2011 09:47:51 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176439</guid>
		<description>What is so special about CaWO4, that makes it a good dark matter detector?</description>
		<content:encoded><![CDATA[<p>What is so special about CaWO4, that makes it a good dark matter detector?</p>
]]></content:encoded>
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		<title>By: Al</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2011/09/05/more-hints-of-dark-matter/comment-page-1/#comment-176236</link>
		<dc:creator>Al</dc:creator>
		<pubDate>Tue, 06 Sep 2011 03:19:50 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/?p=7407#comment-176236</guid>
		<description>Haven&#039;t we been through this about 343 times before?</description>
		<content:encoded><![CDATA[<p>Haven&#8217;t we been through this about 343 times before?</p>
]]></content:encoded>
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