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Study of neutron source reaction 13C(a, n)16O in stars

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Authors

Karakas, Amanda
Li, Zhi-Chang

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China Institute of Atomic Energy

Abstract

13C(α,n)16O is the main neutron source reaction of slow neutron capture (s) process in asymptotic giant branch (AGB) stars. The 6.356 MeV 1/2+ subthreshold resonance in 17O plays an important role in the 13C(α,n)16O reaction. The 13C(11B, 7Li)17O angula

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Source

Yuanzineng Kexue Jishu/Atomic Energy Science and Technology

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Restricted until

2037-12-31