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Microscopic study of radiative fusion reactions 3He(α,γ)7Be and 3H(α,γ)7Li at astrophysical low ENERGIES

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Fusion Reactions Below the Coulomb Barrier

Part of the book series: Lecture Notes in Physics ((LNP,volume 219))

Abstract

Astrophysical S-factor for the reaction 3He(α,γ)7Be, which is one of the key reactions for the solar neutrino problem, is microscopically investigated in terms of the resonating group method. After removing several uncertainties from the theoretical calculation of the S-factor, we obtain a value S = 0.508 keV-barn at Ecm = 10 keV. This value supports a series of the Caltech data.

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Authors and Affiliations

  1. Department of Physics, Faculty of Science, Tokyo Metropolitan University, 2-1-1 Fukazawa, Setagaya-ku, 158, Tokyo, Japan

    Toshitaka Kajino

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  1. Toshitaka Kajino
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S. G. Steadman

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© 1985 Springer-Verlag

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Kajino, T. (1985). Microscopic study of radiative fusion reactions 3He(α,γ)7Be and 3H(α,γ)7Li at astrophysical low ENERGIES. In: Steadman, S.G. (eds) Fusion Reactions Below the Coulomb Barrier. Lecture Notes in Physics, vol 219. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-13918-4_43

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  • DOI: https://doi.org/10.1007/3-540-13918-4_43

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-13918-8

  • Online ISBN: 978-3-540-39146-3

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