@misc{oai:repo.qst.go.jp:00071946,
 author = {Hayakawa, T. and Toh, Y. and Shizuma, T. and Kimura, A. and Nakamura, S. and Harada, H. and Iwamoto, N. and Kajino, T. and 早川 岳人 and 静間 俊行},
 month = {Jun},
 note = {The astrophysical origin of 115Sn has remained still an open question. An isomer with a half-life of 14.1 y at 264 keV in 113Cd is a branching point from which a nucleosynthesis flow reaches to a rare isotope 115Sn. We have measured gamma-rays from neutron capture reactions on an enriched 112Cd target with neutrons provided from an intense neutron beam at ANNRI in J-PARC. We will discuss the contribution of the s-process flow from the 112Cd isomer to the solar abundance of 115Sn, 14th International Symposium on Nuclei in the Cosmos XIV},
 title = {Neutron capture reaction on Cd-112 to study of the s-process origin of Sn-115},
 year = {2016}
}