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...

詳細記述

書誌詳細
主要な著者: Sieverding Andre, Martínez Pinedo Gabriel, Langanke Karlheinz, Harris J. Austin, Hix W. Raphael
フォーマット: 論文
言語:English
出版事項: EDP Sciences 2017-01-01
シリーズ:EPJ Web of Conferences
オンライン・アクセス:https://doi.org/10.1051/epjconf/201716501045