@inproceedings{oai:repo.qst.go.jp:00054934,
 author = {Hayakawa, T. and Kusakabe, K. and Ko, H. and Cheoun, M.-K. and Mathews, G.J. and Tolstov, A. and Nomoto, K. and Chiba, S. and Usang, M. and Hashimoto, M. and Ono, M. and Kajino, T. and Nakamura, T. and Nakamura, K. and Kando, M. and Kotaki, H. and 早川 岳人 and 神門 正城 and 小瀧 秀行},
 book = {Proceedings of the International Symposium on Origin of Matter and Evolution of Galaxies (OMEG 2017)},
 month = {Oct},
 note = {A huge number of neutrinos emitted in core-collapse supernova explosions (neutrino process) play an important role in stellar
nucleosynthesis of some rare nuclides. The study of the neutrino process can contribute to estimation of neutrino energy spectra
and explosion mechanism. In the mass region heavier than iron, only three nuclides are known as the neutrino isotopes. If we can
find other candidates for neutrino production, it helps to constrain precisely the neutrino energy spectra emitted from proto-neutron
stars. A key input for the calculation of the neutrino process is destruction rates by photodisintegration reactions on excited nuclei
at high temperature environments. We have proposed direct measurements of photon-induced reaction cross sections on nuclei
excited by high power laser to simulate stellar environments.},
 pages = {020021-1--020021-6},
 publisher = {American Institute of Physics},
 title = {Neutirno process with primitive meteorites and high power laser},
 volume = {1947},
 year = {2017}
}