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Aspen Dark Matter talk
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Wednesday, February 16, 2011 10:25:42 AM CST
Wednesday, February 16, 2011 10:25:42 AM CST
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  • Indirect Detection of Dark Matter Similar accumulation in Galactic and terrestrial gravitational wells, dwarf spheroidals IceCube can also probe dark matter decay models, other types of dark matter Expected Neutrino Energy Spectrum � All neutrinos from the Sun are low energy for IceCube (few GeV), even for the highest dark matter masses � For Galactic and Earth searches, no significant neutrino energy losses in dense medium, so higher energy neutrinos possible 5 TeV ? 20-25 m in shallower ice) 250 m 350 m Deep Core extra veto cap AMANDA IceCube DeepCore � Eight special strings plus 7 nearest standard IceCube strings � 72 m interstring spacing � 7 m DOM spacing � High Q.E.
  • PMTs � ~5x ...
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Aspen Dark Matter.pdf
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Appears In: Aspen Winter Conference: Dark Matter Detection
Preferred Version: Aspen Dark Matter talk

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