The ν process in the innermost supernova ejecta
The neutrino-induced nucleosynthesis (ν process) in supernova explosions of massive stars of solar metallicity with initial main sequence masses between 13 and 30 M⊙ has been studied with an analytic explosion model using a new extensive set of neutrino-nucleus cross-sections and spectral properties...
主要な著者: | , , , , |
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フォーマット: | 論文 |
言語: | English |
出版事項: |
EDP Sciences
2017-01-01
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シリーズ: | EPJ Web of Conferences |
オンライン・アクセス: | https://doi.org/10.1051/epjconf/201716501045 |