The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model

H. Krauss, K. Grun, T. Rauscher, H. Oberhummer

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Abstract

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

Original languageEnglish
Pages (from-to)258-266
Number of pages9
JournalAnnalen der Physik
Volume2
Issue number3
Publication statusPublished - 1993

Keywords

  • LI-7(N,GAMMA)LI-8
  • SCATTERING
  • NUCLEAR REACTIONS
  • SOLAR NEUTRINOS
  • ASTROPHYSICAL S-FACTOR
  • BE-7(P,GAMMA)B-8
  • CROSS-SECTION

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