Difference between revisions of "Observational Basis for Dark Matter"
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Hoon: Large-scale structure, re-ionization, | Hoon: Large-scale structure, re-ionization, | ||
cosmic microwave background | cosmic microwave background | ||
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+ | ==Presentation== | ||
+ | * [[media:popescu-7-2011.pptx|Observational Basis for Dark Matter]] - powerpoint presentation |
Revision as of 14:04, 2 August 2013
Presentation Files
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? |
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Presentation Outline
Me: Neutralinos, WIMPs, super-symmetry, Detection (experiments)
Hoon: Large-scale structure, re-ionization, cosmic microwave background
Presentation
- Observational Basis for Dark Matter - powerpoint presentation