Predicted solar neutrino rates in the Q-nuclear solar model

Details Predicted solar neutrino rates in the Q-nuclear solar model Predicted solar neutrino rates in the Q-nuclear solar model

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..54..485s&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 54, Feb. 4, 1985, p. 485-487.

Astronomy and Astrophysics

Astronomy

6

Hadrons, Particle Theory, Solar Neutrinos, Astronomical Models, Positrons, Radiation Counters, Radioactive Decay

Scientific paper

It has been shown previously that the existence of a tiny abundance of nuclei which have an additional embedded hadronic particle, Q-nuclei, can solve the solar-neutrino problem. The authors present detailed predictions of solar-neutrino detection rates for detectors of 37Cl, 71Ga, and 115In. It is found that, while Q-nuclei could reduce the 37Cl detection rate from that of the standard model to the experimental value, they would also produce a dramatic increase in the rates for the 71Ga and 115In detectors.

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