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- W2267874503 abstract "The 13C(α,n)16O reaction is believed to be the main neutron source reaction for the s-process in asymptotic giant branch (AGB) stars. The astrophysical S-factors of this reaction have been determined based on an evaluation of the α spectroscopic factor of the 1/2+ subthreshold state in 17O (Ex=6.356 MeV) by using the 13C(11B,7Li)17O α transfer reaction. Our result confirms that the 1/2+ subthreshold resonance is dominant for the 13C(α,n)16O reaction at low energies of astrophysical interest." @default.
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- W2267874503 date "2012-01-01" @default.
- W2267874503 modified "2023-10-17" @default.
- W2267874503 title "Indirect Measurement of Astrophysical 13^C（a, n）^16O S-Factors" @default.
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