Difference between revisions of "Observational Basis for Dark Matter"
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#[http://arxiv.org/PS_cache/arxiv/pdf/1106/1106.2529v1.pdf Actual Evidence] | #[http://arxiv.org/PS_cache/arxiv/pdf/1106/1106.2529v1.pdf Actual Evidence] | ||
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| + | |||
| + | ==Presentation Outline== | ||
| + | Me: Neutralinos, WIMPs, super-symmetry, | ||
| + | Detection (experiments) | ||
| + | |||
| + | Hoon: Large-scale structure, re-ionization, | ||
| + | cosmic microwave background | ||
Revision as of 20:05, 22 July 2011
Background Information on Dark Matter
Questions for Internet Research
| Questions | Sources with Possible Answers |
|---|---|
| 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