Superheavy magnetic monopoles and main-sequence stars

Details Superheavy magnetic monopoles and main-sequence stars Superheavy magnetic monopoles and main-sequence stars

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...335..844f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 335, Dec. 15, 1988, p. 844-861.

Astronomy and Astrophysics

Astrophysics

6

Magnetic Monopoles, Main Sequence Stars, Nuclear Astrophysics, Stellar Evolution, Stellar Interiors, Cartesian Coordinates, Neutrinos, Shock Waves, Solar Neutrinos, Stellar Mass

Scientific paper

The authors investigate the interactions of superheavy monopoles with stars of mass 0.6 - 25 M_sun;. Over the main-sequence lifetime, stars accumulate significant numbers of monopoles less massive than ≅5×1017GeV. Captured monopoles cluster near the stellar center; there they generate heat by annihilating and, possibly, by catalyzing the decay of baryons. Their contribution to the total stellar luminosity, and their effects on the structure of stars, are calculated. It is also argued that all but the strongly magnetic stars will retain a substantial fraction of the monopoles they capture.

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