151. Neutrino self-interaction and MSW effects on the supernova neutrino-process
- Author
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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, and Mathews, Grant J.
- Subjects
Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Solar and Stellar Astrophysics - Abstract
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. Abundances of $^{7}$Li and heavy isotopes $^{92}$Nb, $^{98}$Tc and $^{138}$La are reduced by a factor of 1.5-2.0 by the $\nu$-SI. In contrast, $^{11}$B is relatively insensitive to the $\nu$-SI. We find that the abundance ratio of heavy to light nucleus, $^{138}$La/$^{11}$B, is sensitive to the neutrino mass hierarchy, and the normal mass hierarchy is more likely to be consistent with the solar abundances.
- Published
- 2019
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