The effects of Q-nuclei on stellar burning

Details The effects of Q-nuclei on stellar burning The effects of Q-nuclei on stellar burning

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aipc..126..145b&link_type=abstract

IN: Solar neutrinos and neutrino astronomy; Proceedings of the Conference, Lead, SD, August 23-25, 1984 (A86-37626 17-93). New Y

Physics

Nuclear Physics

1

Nuclear Astrophysics, Nuclear Fusion, Nuclei (Nuclear Physics), Solar Neutrinos, Stellar Models, Abundance, Baryons, Beta Particles, Reaction Kinetics

Scientific paper

The effects of anomalous nuclei, Q-nuclei, on stellar burning are examined. The baryon binding energies, beta-decay properties, and thermonuclear reaction rates for the Q-nuclei suggest they could catalyze a cycle in which four protons are combined to form a 4He nucleus. The properties required of the Q-nuclei for them to solve the solar neutrino problem are determined. A solar modelling calculation was performed with Q-nuclei included, and several interesting results therefrom are compared to observations. Finally the solar neutrino detection rates for 71Ga and 115In detectors, in addition to that for 37Cl, are estimated when Q-nuclei are included in the solar burning.

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