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Measurement of isomer prodcution ratio of 113Cd following neutron capture reactions to investigate origin of 115Sn
https://repo.qst.go.jp/records/58844
https://repo.qst.go.jp/records/5884449310c7c-6906-416a-9bcb-e39170eebc60
Item type | 一般雑誌記事 / Article(1) | |||||
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公開日 | 2018-03-20 | |||||
タイトル | ||||||
タイトル | Measurement of isomer prodcution ratio of 113Cd following neutron capture reactions to investigate origin of 115Sn | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Hayakawa, Takehito
× Hayakawa, Takehito× Shizuma, Toshiyuki× Toh, Yosuke× Huang, Minghui× Kimura, Atsushi× Shoji, Nakamura× Hideo, Harada× Satoshi, Chiba× 早川 岳人× 静間 俊行 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The astrophysical origin of a rare isotope 115Sn has remained still an open question. An isomer (T1=2=14.1 y) in 113Cd is an s-process branching point from which a nucleosynthesis flow reaches to 115Sn. We measured the relative isomer production ratio on 112Cd using neutrons provided from MLF in J-PARC. The result suggests that the contribution of this s-process is not major. | |||||
書誌情報 |
"Annual Report of the National Astronomical Observatory of Japan FY 2016" 発行日 2017-06 |
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関連サイト | ||||||
識別子タイプ | URI | |||||
関連識別子 | https://www.nao.ac.jp/about-naoj/reports/annual-report/en/2016.html | |||||
関連名称 | https://www.nao.ac.jp/about-naoj/reports/annual-report/en/2016.html |