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

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

1993-01-27

arxiv.org/abs/nucl-th/9301018v2

Annalen Phys. 2 (1993) 258-266

Physics

Nuclear Physics

Nuclear Theory

18 pages, 5 figures (available from author on request), Annalen der Physik in press, 1993

Scientific paper

The astrophysical $S$-factor for the reaction $^7$Be(p,$\gamma$)$^8$B up to
an energy of 2~MeV (c.m.) and the capture cross section of
$^7$Li(n,$\gamma$)$^8$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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