The (n, gamma) Cross Section of ^7Li

Details The (n, gamma) Cross Section of ^7Li The (n, gamma) Cross Section of ^7Li

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...507..997h&link_type=abstract

The Astrophysical Journal, Volume 507, Issue 2, pp. 997-1002.

Astronomy and Astrophysics

Astronomy

13

Methods: Laboratory, Nuclear Reactions, Nucleosynthesis, Abundances

Scientific paper

The ^7Li(n, gamma)^8Li reaction has relevance for primordial nucleosynthesis in inhomogeneous big bang models as well as in connection with the solar neutrino problem, where the mirror reaction ^7Be(p, gamma)^8Be is responsible for the production of high-energy solar neutrinos. The cross section was measured at neutron energies of E_n = 5 meV and E_n = 54 keV. With the present results and a reanalysis of a previous measurement, the discrepancies among existing data could be resolved and the cross section can be determined with improved accuracy.

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