Final results on the 13C(α,n)16O cross section at low energies at LUNA
It is well established that the 13C(α, n)16O reaction (Q=2.215 MeV) is the major neutron source feeding the s-process in low mass (1−3M⊙) Asymptotic Giant Branch (AGB) stars. In the last decades, several measurements have been performed. Nevertheless, no dataset reaches the Gamow window (140 keV <Ec...
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| 主要な著者: | , , , , |
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| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
EDP Sciences
2022-01-01
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| シリーズ: | EPJ Web of Conferences |
| オンライン･アクセス: | https://www.epj-conferences.org/articles/epjconf/pdf/2022/04/epjconf_nic16th2022_08003.pdf |
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