Resonating-group calculation of radiative capture reactions (He3,)Be7 and (t,)Li7 at astrophysical low energies

Toshitaka Kajino; Akito Arima

doi:10.1103/PhysRevLett.52.739

Resonating-group calculation of radiative capture reactions (He3,)Be7 and (t,)Li7 at astrophysical low energies

Toshitaka Kajino^*
, Akito Arima

^*此作品的通讯作者

The University of Tokyo

科研成果: 期刊稿件 › 文章 › 同行评审

71 引用（Scopus）

摘要

Total cross sections and astrophysical S factors of the radiative capture reactions (He3,)Be7 and (t,)Li7 are investigated by the resonating-group method. The theoretical value of the S factor at Ec.m.=10 keV is predicted to be 0.508 keVb without the use of any artificial parameters. An interesting difference between the mirror reactions is found and theoretically explained.

源语言	英语
页（从-至）	739-742
页数	4
期刊	Physical Review Letters
卷	52
期	9
DOI	https://doi.org/10.1103/PhysRevLett.52.739
出版状态	已出版 - 1984
已对外发布	是

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10.1103/PhysRevLett.52.739

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引用此

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abstract = "Total cross sections and astrophysical S factors of the radiative capture reactions (He3,)Be7 and (t,)Li7 are investigated by the resonating-group method. The theoretical value of the S factor at Ec.m.=10 keV is predicted to be 0.508 keVb without the use of any artificial parameters. An interesting difference between the mirror reactions is found and theoretically explained.",

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AB - Total cross sections and astrophysical S factors of the radiative capture reactions (He3,)Be7 and (t,)Li7 are investigated by the resonating-group method. The theoretical value of the S factor at Ec.m.=10 keV is predicted to be 0.508 keVb without the use of any artificial parameters. An interesting difference between the mirror reactions is found and theoretically explained.

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