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The Astrophysical S-Factor of the Reaction $^7$be(p,$γ$)$^8$B in the Direct Capture Model

H. Krauss·K. Gr"un·T. Rauscher·H. Oberhummer
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Abstract

The astrophysical $S$-factor for the reaction $^7$Be(p,$γ$)$^8$B up to an energy of 2~MeV (c.m.) and the capture cross section of $^7$Li(n,$γ$)$^8$Li up to 1~MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.

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H. Krauss, K. Gr"un, T. Rauscher, H. Oberhummer. 1993-01-28. The Astrophysical S-Factor of the Reaction $^7$be(p,$γ$)$^8$B in the Direct Capture Model. https://doi.org/10.1002/andp.19935050304

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