A Classical Instability of Reissner-Nordstrom Solutions and the Fate of Magnetically Charged Black Holes
K. Lee, V. P. Nair, E. J. Weinberg
Abstract
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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