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Observational Basis for Dark Matter (view source)
Revision as of 14:32, 25 July 2011
, 14:32, 25 July 2011→Questions for Internet Research
|3. What are the properties of WIMPs, and how can they be detected?
|3. What are the properties of WIMPs, and how can they be detected?
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#[http://en.wikipedia.org/wiki/Neutralino The Neutralino]
#[http://en.wikipedia.org/wiki/Neutralino The Neutralino] ''Starting Point '''not reliable''' ''
#[http://en.wikipedia.org/wiki/Weakly_interacting_massive_particles WIMP Detection]
#[http://en.wikipedia.org/wiki/Weakly_interacting_massive_particles WIMP Detection] ''Starting Point '''not reliable''' ''
#[http://cdms.berkeley.edu/Education/DMpages/science/directDetection.shtml Direct Detection]
#[http://cdms.berkeley.edu/Education/DMpages/science/directDetection.shtml Direct Detection] ''General Information '''not reliable''' ''
#[http://www.astro.princeton.edu/~dns/MAP/Bahcall/node14.html Solar WIMP Detection]
#[http://www.astro.princeton.edu/~dns/MAP/Bahcall/node14.html Solar WIMP Detection] '''Reliable'''
#[http://web.mit.edu/~redingtn/www/netadv/specr/6/node7.html Antarctic Neutrino Detection]
#[http://web.mit.edu/~redingtn/www/netadv/specr/6/node7.html Antarctic Neutrino Detection] '''Reliable'''
#[http://arxiv.org/PS_cache/astro-ph/pdf/0211/0211500v1.pdf Direct Detection Techniques]
#[http://arxiv.org/PS_cache/astro-ph/pdf/0211/0211500v1.pdf Direct Detection Techniques] ''Specific detector information '''Reliable''' ''
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