Neutrino self-interaction and MSW effects on the supernova neutrino-process

23 Nov 2019 Ko Heamin Cheoun Myung-Ki Ha Eunja Kusakabe Motohiko Hayakawa Takehito Sasaki Hirokazu Kajino Toshitaka Hashimoto Masa-aki Ono Masaomi Usang Mark D. Chiba Satoshi Nakamura Ko Tolstov Alexey Nomoto Ken'ichi Kawano Toshihiko Mathews Grant J.

We calculate the abundances of $^{7}$Li, $^{11}$B, $^{92}$Nb, $^{98}$Tc, $^{138}$La, and $^{180}$Ta produced by neutrino $(\nu)$ induced reactions in a core-collapse supernova explosion. We consider the modification by $\nu$ self-interaction ($\nu$-SI) near the neutrinosphere and the Mikheyev-Smirnov-Wolfenstein effect in outer layers for time-dependent neutrino energy spectra... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • SOLAR AND STELLAR ASTROPHYSICS