baboons
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baboons [2014/06/09 17:36] cook |
baboons [2014/06/09 17:58] cook |
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| - The abundance of X. | - The abundance of X. | ||
| - n interaction rates with every other nucleus. | - n interaction rates with every other nucleus. | ||
| + | - Mass of the WIMP. Chosen to be 100 GeV, based on the wikipedia WIMP entry, the font of all wisdom. | ||
| + | This figure: | ||
| + | {{::cdms_parameter_space_2004.png?300|}} | ||
| + | |||
| + | from CDMS in 2004 suggests that this value isn't too far off. | ||
| Reference Papers: | Reference Papers: | ||
| - | Cyburt et. al. 2009 Nucleosynthesis Constraints on a Massive Gravitino in Neutralino Dark Matter Scenario [[http://arxiv.org/pdf/0907.5003v1.pdf]] | + | Cyburt et. al. 2009. Nucleosynthesis Constraints on a Massive Gravitino in Neutralino Dark Matter Scenario [[http://arxiv.org/pdf/0907.5003v1.pdf]] |
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| + | |||
| + | Kamionkowski 1994. Diffuse Gamma Rays from WIMP Decay and Annihilation [[http://arxiv.org/pdf/astro-ph/9404079v1.pdf]] | ||
| **Logbook** | **Logbook** | ||
baboons.txt · Last modified: 2014/06/13 10:24 by cook
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