Neutrino Astronomy in the TeV to PeV Energy Range
碩士 === 國立交通大學 === 物理研究所 === 95 === We examine the prompt and conventional atmospheric neutrino fluxes where different models for the prompt flux are employed. Due to different angular dependencies between the prompt flux and the conventional ones, we compare the shower event ratio due to the prompt...
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| Format: | Others |
| Language: | en_US |
| Published: |
2007
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| Online Access: | http://ndltd.ncl.edu.tw/handle/84221106913781467223 |
| Summary: | 碩士 === 國立交通大學 === 物理研究所 === 95 === We examine the prompt and conventional atmospheric neutrino fluxes where different models for the prompt flux are employed. Due to different angular dependencies between the prompt flux and the conventional ones, we compare the shower event ratio due to the prompt flux to that due to the conventional flux. This is important to separate the prompt atmospheric neutrino flux from the conventional component. The determination of the former is useful for testing the models for charm productions.
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