Energy loss of supermassive magnetic monopoles and dyons in main sequence stars

Details Energy loss of supermassive magnetic monopoles and dyons in main sequence stars Energy loss of supermassive magnetic monopoles and dyons in main sequence stars

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrvd..55.6584a&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 55, Issue 10, 15 May 1997, pp.6584-6590

Physics

1

Magnetic Monopoles, Energy Loss And Stopping Power, Normal Stars : General Or Individual

Scientific paper

We estimate the energy loss rate for a supermassive magnetic monopole or dyon in the interior of a main sequence star. For this purpose, the medium is shown to behave as a nondegenerate classical electron gas, the nuclear contribution to the stopping power being negligible. A linear dependence of the energy loss from the velocity of the particle is obtained. This result would provide a basic input to detailed calculations of the dynamics of monopoles and dyons in our galaxy.

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