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Deformations of the Schwarzschild Black Hole

D. Grumiller
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Abstract

Due to its large number of symmetries the Schwarzschild Black Hole can be described by a specific two-dimensional dilaton gravity model. After reviewing classical, semi-classical and quantum properties and a brief discussion of virtual black holes deformations are studied: the first part is devoted to deformations of the Lorentz-symmetry, the second part to dynamical deformations and its role for the long time evaporation of the Schwarzschild Black Hole.

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D. Grumiller. 2003-12-18. Deformations of the Schwarzschild Black Hole. https://arxiv.org/abs/gr-qc/0311011

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