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

1991-11-22

arxiv.org/abs/hep-th/9111045v2

Phys.Rev.Lett. 68 (1992) 1100-1103

Physics

High Energy Physics

High Energy Physics - Theory

(10 pages)

Scientific paper

10.1103/PhysRevLett.68.1100

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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