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

Preprint

27 January 1993

preprint
Published by arXiv in arXiv

Abstract

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.

Keywords

DIRECT CAPTURE
CROSS SECTION
ASTROPHYSICAL
CAPTURE MODEL
CAPTURE CROSS
GAMMA
MEV
C.M

All Related Versions

Version 1, 1993-01-27, ArXiv
Version 2, 1993-01-28, ArXiv
Published version: Annalen der Physik, 505 (3), 258.

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