Axion Emissivity from the Conversion of a Neutron Star into a Strange Star

Details Axion Emissivity from the Conversion of a Neutron Star into a Strange Star Axion Emissivity from the Conversion of a Neutron Star into a Strange Star

1998-04-08

arxiv.org/abs/astro-ph/9804091v1

Phys.Lett. B432 (1998) 145-150

Astronomy and Astrophysics

Astrophysics

12 pages, 2 figures, submitted to Phys. Lett. B

Scientific paper

10.1016/S0370-2693(98)00597-8

The conversion of neutron matter into strange matter in a neutron star occurs
through the non-leptonic weak-interaction process. We study the energy loss of
the neutron star by the emission of axions in that process. Owing to that
process, the neutron star will liberate the energy which can in no way be
negligible as an axion burst.

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