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Evaluation of neutron capture cross section on 205Pb with photonuclear data
https://repo.qst.go.jp/records/54913
https://repo.qst.go.jp/records/5491308697daf-1d65-4524-8830-6725d87f4cd3
Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-06-07 | |||||
タイトル | ||||||
タイトル | Evaluation of neutron capture cross section on 205Pb with photonuclear data | |||||
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_5794 | |||||
資源タイプ | conference paper | |||||
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 |
岩本信之
× 岩本信之× 静間, 俊行× 静間 俊行 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | The neutron capture cross section of long-lived radioactive 205Pb is derived by using the nuclear reaction calculation code CCONE, based on photonuclear data. The present result is smaller than that of TENDL-2015 by a factor of 4. The derived Maxwellian averaged capture cross section (MACS) is the smallest compared to the existing data. The produced amount of 205Pb is explored with a simulated neutron flux in the Pb-Bi eutectic (LBE) target. The continuous use of the system in 25 years creates 205Pb with about 6 kg at maximum in the LBE (including natural Pb of 103 kg). The impact of the derived MACS on the stellar nucleosynthesis is investigated. It is found that the abundance of Tl is slightly enhanced due to the increase in the remaining abundance of 205Pb. | |||||
書誌情報 |
EPJ Web Conf 巻 178, p. 06004, 発行日 2018-05 |
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DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1051/epjconf/201817806004 | |||||
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識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1051/epjconf/201817806004 | |||||
関連名称 | https://doi.org/10.1051/epjconf/201817806004 |