Improved Calculation of non-fusion Solar Neutrinos Produced by Rubakov Effects.

Details Improved Calculation of non-fusion Solar Neutrinos Produced by Rubakov Effects. Improved Calculation of non-fusion Solar Neutrinos Produced by Rubakov Effects.

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jkas...26...79l&link_type=abstract

Journal of the Korean Astronomical Society, vol. 26, no. 1, p. 79-81

Astronomy and Astrophysics

Astronomy

Monopole, Solar Neutrinos

Scientific paper

We calculated the solar monopole abundance limit by comparing the observed solar neutrino flux and the calculation of non-fusion solar neutrino flux produced by Rubakov process in the solar core. We included the produced meson's enhancement effects by the surrounding ions in the solar core. We find that the monopole number N_m < 1.9*10E20 (1 mb/sigma_0), where sigma_0 is the characteristic proton decay cross section of Rubakov process. This is similar or stronger than strong limits obtained from neutron star's luminosity.

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