The fate of magnetically charged black holes

Details The fate of magnetically charged black holes The fate of magnetically charged black holes

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992gregr..24.1203l&link_type=abstract

General Relativity and Gravitation, Volume 24, Issue 12, pp.1203-1207

Computer Science

7

Scientific paper

The magnetically charged Reissner-Nordström black hole solutions of Maxwell-Einstein theory cannot evaporate completely, because their Hawking temperature tends to zero as their mass to charge ratio approaches unity. This situation changes when these solutions are considered in the context of a non-Abelian gauge theory containing nonsingular magnetic monopoles. If the horizon is sufficiently small, the Reissner-Nordström solution develops a classical instability and evolves into a new type of magnetically charged black hole solution. The temperature of these new solutions increases monotonically as the horizon contracts, so that there is no obstacle to the complete evaporation of a magnetically charged black hole.

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