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Nuclear cosmochronometer for supernova neutrino process
https://repo.qst.go.jp/records/76486
https://repo.qst.go.jp/records/76486ba9f8a04-4693-4020-b85d-46a8450f694d
| Item type | 会議発表用資料 / Presentation(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2019-06-24 | |||||
| タイトル | ||||||
| タイトル | Nuclear cosmochronometer for supernova neutrino process | |||||
| 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_c94f | |||||
| 資源タイプ | conference object | |||||
| 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× Kusakabe, M.× Kajino, T.× Cheoun, M.K.× Ko, H.× Mathews, G.J.× Tolstov, A.× Nomoto, K.× Chiba, S.× Kawano, T,× Ono, M.× Hayakawa, Takehito |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | Short-lived radioisotopes with half-lives of 0.1-10 Myr are known as nuclear cosmochronometers to evaluate the passing time from a nucleosynthesis event such as s-process in an AGB star or r-process to the solar system formation (SSF). Neutron rich short-lived radioisotopes such as 129I and 244Pu, which were predominantly produced by the r process, have been studied in order to evaluate the age of the last supernova (SN) around the solar system. However, the recent studies show neutron star mergers are a candidate for the r process. Thus, there is no robust cosmic clock for the last SN before the SSF. We focus our attention on neutron-deficient short-lived radioisotopes, in particular, which may be produced by neutrino-process. This is because the neutrino process can occur only in core-collapse SNe. In an early phase, a huge number of neutrinos are emitted from a proto neutron star formed in the center of a massive star. Some neutrinos interact with preexisting isotopes and thereby produce rare neutron deficient isotopes such as 138 La, and 180Ta as well as 7Li and 11B. There are five neutrino-deficient short-lived isotopes of 53Mn, 92Nb, 97Tc, 98Tc, 146Sm. We have proposed the neutrino-process origin for unstable isotopes for 92Nb (T1/2=35 Myr) and 98Tc (T1/2=4.2 Myr). We have calculated neutrino-induced reaction cross section involved using the QRPA model and statistical model. We have calculated the neutrino-isotope abundances in SNe using SN models. In the case of 92Nb, its initial abundance at SSF could be reproduced by the later input model. It is found that it is possible to explain the origin of 92Nb by the SN neutrino process. In contrast, for 98Tc, the upper limit for the initial abundance was reported. The calculated result is consistent with the observed upper limit. We discuss possible age for the last SN for various neutrino process chronometers. |
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| 会議概要（会議名, 開催地, 会期, 主催者等） | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | The 15th International Symposium on Origin of Matter and Evolution of Galaxies | |||||
| 発表年月日 | ||||||
| 日付 | 2019-07-04 | |||||
| 日付タイプ | Issued | |||||
