P-P chain non-resonant reactions with a quasi non-degenerate distribution

Details P-P chain non-resonant reactions with a quasi non-degenerate distribution P-P chain non-resonant reactions with a quasi non-degenerate distribution

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..214a&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

Computer Science

Maxwell-Boltzmann Density Function, Radiation Counters, Solar Neutrinos, Thermonuclear Reactions, Abundance, Main Sequence Stars, Nucleons

Scientific paper

By using Clayton's (1974) approach, a quasi-nondegenerate distribution (QNDD) has been designed to account for a high solar neutrino counting rate for Cl-37. The QNDD is examined here in the context of certain P-P chain nonresonant reactions of main-sequence stars, with the sun representing a typical case. The results are then compared with the results based on the Maxwell-Boltzmann distribution.

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