Difference between revisions of "Observational Basis for Dark Matter"
Jump to navigation
Jump to search
(2 intermediate revisions by 2 users not shown) | |||
Line 1: | Line 1: | ||
+ | ==Presentation Files== | ||
+ | [http://zeus.phys.uconn.edu/wiki/images/Alex_Popescu_Dark_Matter.pptx Download Version 1.0] | ||
+ | |||
==Background Information on Dark Matter== | ==Background Information on Dark Matter== | ||
===Useful Links=== | ===Useful Links=== | ||
Line 68: | Line 71: | ||
Hoon: Large-scale structure, re-ionization, | Hoon: Large-scale structure, re-ionization, | ||
cosmic microwave background | cosmic microwave background | ||
+ | |||
+ | ==Presentation== | ||
+ | * [[media:popescu-7-2011.pptx|The Other Side of the Universe: Dark Matter]] - powerpoint presentation |
Latest revision as of 14:05, 2 August 2013
Presentation Files
Background Information on Dark Matter
Useful Links
Questions for Internet Research
Questions | Sources with Possible Answers |
---|---|
1. How can we be sure dark matter exists? |
|
2. What are the possible candidates for the particles that actually make up dark matter? |
|
3. What are the properties of WIMPs, and how can they be detected? |
|
4. What ongoing research is being done to detect and experiment with dark matter? |
|
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
Presentation
- The Other Side of the Universe: Dark Matter - powerpoint presentation