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    <title>lux</title>
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  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>The concept of dark matter arose as a solution to a problem that has been puzzling astronomers for decades. Galaxies, when observed, rotate at a much faster rate than is expected for the estimated mass they contain.....</abstract>
</record>

<record>
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    <title>nasa</title>
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  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Dark Energy, Dark Matter</abstract>
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<record>
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    <title>dark atom</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>New Kind of Dark Matter Could Form 'Dark Atoms'</abstract>
</record>

<record>
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  <titles>
    <title>other than baryons</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Dark matter is the name we give to matter we can not observe directly, and that appears to be made up of something other than baryons.</abstract>
</record>

<record>
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  <titles>
    <title>Dark Matter Matters, Especially When You Can't Find It</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>http://news.discovery.com/space/galaxies/hubble-space-telescope-latest-cosmic-pictures-130129.htm</abstract>
</record>

<record>
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  <titles>
    <title>The Alpha Magnetic Spectrometer (AMS)</title>
    <secondary-title/>
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  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Dark matter is thought to make up 80 percent of all matter in the Universe, the rest is “baryonic matter” — i.e. the stuff we’re made of. But the vast majority of matter is locked in an invisible component of matter. As the moniker suggests, dark matter is dark; it doesn’t interact with electromagnetic radiation. However, dark matter still carries mass that has a gravitational effect on space-time and through indirect means we can detect its gravitational presence. ..</abstract>
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    <title>mma dm</title>
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    <year/>
  </dates>
  <abstract>mm dm detection</abstract>
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<record>
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  <titles>
    <title>snowmass</title>
    <secondary-title/>
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  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>Snowmass Working Group Reports</abstract>
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<record>
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  <titles>
    <title>snowmass13</title>
    <secondary-title/>
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  <dates>
    <year/>
  </dates>
  <abstract>Contributed Papers Submitted to the Snowmass 2013 Study
&lt;br /&gt;</abstract>
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<record>
  <contributors/>
  <titles>
    <title>Dark and Darker:  The Search for Dark Matter and Dark Energy-2005</title>
    <secondary-title/>
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  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>http://www.astro.caltech.edu/~golwala/talks/20050521CaltechSeminarDay.pdf</abstract>
</record>

<record>
  <contributors/>
  <titles>
    <title>SM and DM</title>
    <secondary-title/>
  </titles>
  <doi/>
  <pages/>
  <volume/>
  <number/>
  <dates>
    <year/>
  </dates>
  <abstract>The Standard Model (SM) of particle physics fails to explain dark matter and why matter survived annihilation with antimatter following the Big Bang. Extensions to the SM, such as weak-scale Supersymmetry, may explain one or both of these phenomena by positing the existence of new particles and interactions that are asymmetric under time-reversal (T).</abstract>
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