Difference between revisions of "Observational Basis for Dark Matter"
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| + | ==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=== | ||
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#[http://content.lib.utah.edu/cdm4/document.php?CISOROOT=/ir-main&CISOPTR=34624 Science Papers] '''Reliable''' | #[http://content.lib.utah.edu/cdm4/document.php?CISOROOT=/ir-main&CISOPTR=34624 Science Papers] '''Reliable''' | ||
#[http://www.phy.ncu.edu.tw/hep/inc/NCU04AST.pdf Indirect Neutrino Detection] ''Good pictures '''not reliable''' '' | #[http://www.phy.ncu.edu.tw/hep/inc/NCU04AST.pdf Indirect Neutrino Detection] ''Good pictures '''not reliable''' '' | ||
| − | #[http://mckinseygroup.physics.yale.edu/Publications/MiniCLEAN_McKinsey.pdf MiniCLEAN Experiment] | + | #[http://mckinseygroup.physics.yale.edu/Publications/MiniCLEAN_McKinsey.pdf MiniCLEAN Experiment] ''Good pictures '''Not Reliable''' '' |
#[http://www.ifm.umich.mx/~raya/papers/AIP-CP1026-195-2008.pdf Ongoing Research] '''Reliable''' | #[http://www.ifm.umich.mx/~raya/papers/AIP-CP1026-195-2008.pdf Ongoing Research] '''Reliable''' | ||
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|5. Where do we think all the super-symmetric particles are? | |5. Where do we think all the super-symmetric particles are? | ||
| | | | ||
| − | #[http://en.wikipedia.org/wiki/Supersymmetry Super-symmetric Particles] | + | #[http://en.wikipedia.org/wiki/Supersymmetry Super-symmetric Particles] ''Good background information and Links, '''not reliable''' '' |
| − | #[http://www.weizmann.ac.il/particle/nir/uploads/file/chapter8.pdf Different SS Particles] | + | #[http://www.weizmann.ac.il/particle/nir/uploads/file/chapter8.pdf Different SS Particles] '''Not reliable''' |
| − | #[http://www.phys.uu.nl/~prokopec/RobertKnegjens_dm2.pdf Explanation of SS Particles] | + | #[http://www.phys.uu.nl/~prokopec/RobertKnegjens_dm2.pdf Explanation of SS Particles] '''Reliable''' |
#[http://arxiv.org/PS_cache/arxiv/pdf/1106/1106.2529v1.pdf Actual Evidence] '''Reliable''' | #[http://arxiv.org/PS_cache/arxiv/pdf/1106/1106.2529v1.pdf Actual Evidence] '''Reliable''' | ||
| + | #[http://arxiv.org/PS_cache/arxiv/pdf/1102/1102.4585v1.pdf Possibility of Super-symmetric particles at LHC] '''Reliable''' | ||
|} | |} | ||
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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