@inproceedings{oai:repo.qst.go.jp:00079706,
 author = {Ko, Heamin and Myung-Ki, Cheoun and Kusakabe, Motohiko and Hayakawa, Takehito and Sasaki, Hirokazu and Kajino, Toshitaka and J. Mathews, Grant and Hayakawa, Takehito},
 book = {JPS Conference Proceedings},
 month = {Mar},
 note = {We investigate nuclear abundances produced from the neutrino neutrino-process in supernova explosions. By adopting an equi-partitioned neutrino-luminosity for each neutrino flavor, we have calculated the neutrino-
flux propagation including both its modification by neutrino self-interaction (neutrino-SI) near the neutrino-sphere and the Mikheyev-Smirnov-Wolfenstein (MSW) effect in the outer O-Ne-Mg layer. The abundances of heavier
isotopes 92Nb, 98Tc and 138La are largely enhanced by the neutrino-SI for the inverted mass hierarchy. The ratio of 7Li/11B is lower in the inverted hierarchy than in the normal hierarchy.},
 publisher = {JPS},
 title = {Neutrino self-interaction and MSW eects by an equi-partitioned Fermi-Dirac neutrino luminosity on the supernova neutrino-process},
 volume = {31},
 year = {2020}
}