Difference between revisions of "Observational Basis for Dark Matter"
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#[http://en.wikipedia.org/wiki/Lightest_Supersymmetric_Particle Neutralinos] ''starting point '''not reliable''' '' | #[http://en.wikipedia.org/wiki/Lightest_Supersymmetric_Particle Neutralinos] ''starting point '''not reliable''' '' | ||
#[http://www.astro.princeton.edu/~dns/MAP/Bahcall/node16.html Axions] ''Very abstract string theory explanation '''Reliable''' '' | #[http://www.astro.princeton.edu/~dns/MAP/Bahcall/node16.html Axions] ''Very abstract string theory explanation '''Reliable''' '' | ||
− | + | #[http://www.ifm.umich.mx/~raya/papers/AIP-CP1026-195-2008.pdf Experiment discussion] '''Reliable''' | |
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Revision as of 14:36, 25 July 2011
Background Information on Dark Matter
Useful Links
Questions for Internet Research
Questions | Sources with Possible Answers |
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1. How can we be sure dark matter exists? |
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2. What are the possible candidates for the particles that actually make up dark matter? |
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3. What are the properties of WIMPs, and how can they be detected? |
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4. What ongoing research is being done to detect and experiment with dark matter? |
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5. Where do we think all the super-symmetric particles are? |
Presentation Outline
Me: Neutralinos, WIMPs, super-symmetry, Detection (experiments)
Hoon: Large-scale structure, re-ionization, cosmic microwave background