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- W201876819 abstract "One possible source of neutrons for the astrophysical {ital s} process is the {sup 22}Ne({alpha},{ital n}){sup 25}Mg reaction. However, the number of neutrons available to synthesize heavy elements may be limited by the rate of the {sup 22}Ne({ital n},{gamma}){sup 23}Ne reaction. To aid in the interpretation of recent ({ital n},{gamma}) measurements, we have used the {sup 22}Ne({ital d},{ital p}){sup 23}Ne reaction to investigate the single-particle structure of states located near the {sup 22}Ne+{ital n} threshold. No states that correspond to astrophysically significant resonances were found, and so the ({ital n},{gamma}) rate is effectively determined by direct capture." @default.
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- W201876819 date "1990-12-01" @default.
- W201876819 modified "2023-09-24" @default.
- W201876819 title "Ne22(d,p)23Ne reaction and neutron balance in thesprocess" @default.
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- W201876819 doi "https://doi.org/10.1103/physrevc.42.2730" @default.
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