The fate of magnetically charged black holes View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1992-12

AUTHORS

Kimyeong Lee, V. P. Nair, Erick J. Weinberg

ABSTRACT

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. More... »

PAGES

1203-1207

References to SciGraph publications

  • 1975-08. Particle creation by black holes in COMMUNICATIONS IN MATHEMATICAL PHYSICS
  • 1975-10. Vacuum polarization and the spontaneous loss of charge by black holes in COMMUNICATIONS IN MATHEMATICAL PHYSICS
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/bf02418208

    DOI

    http://dx.doi.org/10.1007/bf02418208

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1013263346


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