@misc{oai:repo.qst.go.jp:00065937,
 author = {Hayakawa, Takehito and Nakamura, Ko and Kusakabe, Motohiko and Kajino, Toshitaka and Chiba, Satoshi and Iwamoto, Nobuyuki and Cheoun, Myung-Ki and J, Mathews Grant and 早川 岳人},
 month = {Sep},
 note = {We have proposed the neutrino-process origin for 92Nb and reproduced the 92Nb abundance by SN models with assumed neutrino temperatures. Since the neutrino-nucleus interactions are one of key physics, we have calculated them by using QRPA models. We also suggest the possibility that 98Tc (T1/2=4.2 Myr) can be produced by the neutrino process. When the 98Tc abundance at SSF will be measured, we can constrain strongly neutrino temperatures., The 26th International Nuclear Physics Conference},
 title = {Supernova Neutrino Process And Sensitivity To Neutrino Temperatures},
 year = {2016}
}