Dark Matter Induced Mikheyev-Smirnov-Wolfenstain Effect in The Sun And Core-Collapse Supernovae
碩士 === 國立清華大學 === 物理系 === 103 === We studied the dark matter induced Mikheyev-Smirnov-Wolfenstein eect on neutrino oscillations in the Sun and the core-collapse supernovae. However, to have sizable eect, we found that the dark matter cannot self-annihilate, for instance, the asymmetric dark matter....
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| Format: | Others |
| Language: | en_US |
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2015
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| Online Access: | http://ndltd.ncl.edu.tw/handle/19981466588916180420 |
| Summary: | 碩士 === 國立清華大學 === 物理系 === 103 === We studied the dark matter induced Mikheyev-Smirnov-Wolfenstein eect on neutrino oscillations in the Sun and the core-collapse supernovae. However, to have sizable eect, we found that the dark matter cannot self-annihilate, for instance, the asymmetric dark matter. From the solar neutrino data, we found strong constraint on the interaction between dark matter and neutrino for asymmetric dark matter with mass less than 40 GeV. For supernovae, we found that the additional eect would be detectable only if the supernova sits close to the Galactic center or the interaction between dark matter and neutrinos is strong enough.
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