A classical instability of Reissner-Nordstrom solutions and the fate of magnetically charged black holes
Working in the context of spontaneously broken gauge theories, it is shown 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...
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Veröffentlicht in: | Physical review letters 1992-02, Vol.68 (8), p.1100-1103 |
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creator | Lee, Kimyeong Nair, V. P. Weinberg, Erick J. |
description | Working in the context of spontaneously broken gauge theories, it is shown 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. |
doi_str_mv | 10.1103/PhysRevLett.68.1100 |
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P.</creatorcontrib><creatorcontrib>Weinberg, Erick J.</creatorcontrib><title>A classical instability of Reissner-Nordstrom solutions and the fate of magnetically charged black holes</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>Working in the context of spontaneously broken gauge theories, it is shown 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. 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subjects | Astrophysics Classical general relativity Exact sciences and technology General relativity and gravitation Physics |
title | A classical instability of Reissner-Nordstrom solutions and the fate of magnetically charged black holes |
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