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  Instability of the extreme Kerr-Newman black-holes

Reiris, M. (in preparation). Instability of the extreme Kerr-Newman black-holes.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-FE41-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-FE42-3
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1311.3156.pdf (Preprint), 353KB
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 Creators:
Reiris, Martin1, Author              
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1Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24012              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Mathematics, Differential Geometry, math.DG
 Abstract: Using black-hole inequalities and the increase of the horizon's areas, we show that there are arbitrarily small electro-vacuum perturbations of the standard initial data of the extreme Reissner-Nordstrom black-hole that, (by contradiction), cannot decay in time into any extreme Kerr-Newman black-hole. This proves the expectation that the family of extreme Kerr-Newman black-holes is unstable. It remains of course to be seen whether the whole family of charged black-holes, including those extremes, is stable or not.

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 Dates: 2013-11-13
 Publication Status: Not specified
 Pages: 25 pages. 6 figures
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 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1311.3156
URI: http://arxiv.org/abs/1311.3156
 Degree: -

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