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Geometric Inequalities for Black Holes

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Relativity and Gravitation

Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 157))

Abstract

It is well known that the parameters that characterize the Kerr black hole satisfy several important geometric inequalities. Remarkably enough, some of these inequalities also hold for dynamical black holes. This kind of inequalities play an important role in the characterization of the gravitational collapse, they are closely related with the cosmic censorship conjecture. We briefly review recent results in this subject.

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References

  1. Wald, R.M.: Final states of gravitational collapse. Phys. Rev. Lett. 26, 1653 (1971). doi:10.1103/PhysRevLett.26.1653

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  2. Dain, S.: Geometric inequalities for axially symmetric black holes. Class. Quantum Grav. 29, 073001 (2012). doi:10.1088/0264-9381/29/7/073001

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Correspondence to Sergio Dain .

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© 2014 Springer International Publishing Switzerland

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Dain, S. (2014). Geometric Inequalities for Black Holes. In: Bičák, J., Ledvinka, T. (eds) Relativity and Gravitation. Springer Proceedings in Physics, vol 157. Springer, Cham. https://doi.org/10.1007/978-3-319-06761-2_7

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