A classical instability of Reissner-Nordstrom solutions and the fate of magnetically charged black holes

Details A classical instability of Reissner-Nordstrom solutions and the fate of magnetically charged black holes A classical instability of Reissner-Nordstrom solutions and the fate of magnetically charged black holes

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9217697l&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Gauge Theory, Magnetic Monopoles, Reissner-Nordstrom Solution, Electromagnetic Fields, Gravitation, Stellar Evolution

Scientific paper

Working in the context of spontaneously broken gauge theories, we show that the magnetically charged Reissner-Nordstrom solution develops a classical instability if the horizon is sufficiently small. This instability has significant implications for the evolution of a magnetically charged black hole. In particular, it leads to the possibility that such a hole could evaporate completely, leaving in its place a nonsingular magnetic monopole.

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