On the fate of superheavy magnetic monopoles in a neutron star

Physics

Scientific paper

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Scientific paper

We propose two possible scenarios of the behaviour of superheavy magnetic monopoles in a neutron star, in which the monopole-antimonopole annihilation rate is sufficiently large to prevent the enormous heating of a neutron star due to the monopole induced neutron decays. We find that the galactic monopole flux of order 10-16 cm-2 s-1 sterad-1 can be compatible with the observational limit on the X-ray luminosity of neutron stars.
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