Solar monopoles and terrestrial neutrinos

Details Solar monopoles and terrestrial neutrinos Solar monopoles and terrestrial neutrinos

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esna.conf.....f&link_type=abstract

Presented at the Extra Solar Neutrino Astronomy Workshop, Los Angeles, Calif., 30 Sep. 1987

Astronomy and Astrophysics

Astronomy

Detection, Magnetic Monopoles, Neutron Flux Density, Solar Neutrinos, Annihilation Reactions, Neutron Cross Sections, Neutron Stars

Scientific paper

Magnetic monopoles captured in the core of the sun may give rise to a substantial flux of energetic neutrinos by catalyzing the decay of solar hydrogen. We discuss the expected neutrino flux in underground detectors under different assumptions about solar interior conditions. Although a monopole flux as low as FM approximately 10 to the -24/cm/sec/sr/sup could give rise to a neutrino flux above atmospheric background, due to M/bar M/ annihilation, this does not translate into a reliable monopole flux bound stronger than the Parker limit.

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