Constraints on the topology of higher-dimensional black holes

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Abstract

Introduction As discussed in the first chapter, black holes in four dimensions satisfy remarkable uniqueness properties. Of fundamental importance is the classical result of Carter, Hawking and Robinson that the Kerr solution, which is characterized by its mass <italic>M</italic> and angular momentum <italic>J</italic>, is the unique four-dimensional asymptotically flat stationary (i.e., steady state) solution to the vacuum Einstein equations. A basic step in the proof is Hawking's theorem on the topology of black holes [2], which asserts that, for such black hole spacetimes, cross sections of the event horizon are necessarily spherical, i.e., they are topologically 2-spheres. In short, for conventional black holes in four dimensions, the horizon topology is spherical. However, as we saw in the previous chapter, in higher dimensions black hole horizons need not have spherical topology. With the remarkable discovery by Emparan and Reall [3] of the black ring solution, with its S1 × S2 horizon topology, the question naturally arose as to what, if any, are the restrictions on horizon topology in higher-dimensional black holes. This issue was addressed in a paper of the author and Rick Schoen [4], in which we obtained a generalization of Hawking's theorem to higher dimensions. This generalization is discussed in sections 7.4 and 7.5. In preparation for that, we review Hawking's black hole topology theorem in section 7.2 and introduce some basic background material on marginally trapped surfaces in section 7.3.

Original languageEnglish (US)
Title of host publicationBlack Holes in Higher Dimensions
PublisherCambridge University Press
Pages159-179
Number of pages21
ISBN (Print)9781139004176, 9781107013452
DOIs
StatePublished - Jan 1 2012

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topology
horizon
theorems
event horizon
Einstein equations
uniqueness
constrictions
angular momentum
momentum
vacuum
preparation
rings
cross sections

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Galloway, G. J. (2012). Constraints on the topology of higher-dimensional black holes. In Black Holes in Higher Dimensions (pp. 159-179). Cambridge University Press. https://doi.org/10.1017/CBO9781139004176.008

Constraints on the topology of higher-dimensional black holes. / Galloway, Gregory J.

Black Holes in Higher Dimensions. Cambridge University Press, 2012. p. 159-179.

Research output: Chapter in Book/Report/Conference proceedingChapter

Galloway, GJ 2012, Constraints on the topology of higher-dimensional black holes. in Black Holes in Higher Dimensions. Cambridge University Press, pp. 159-179. https://doi.org/10.1017/CBO9781139004176.008
Galloway GJ. Constraints on the topology of higher-dimensional black holes. In Black Holes in Higher Dimensions. Cambridge University Press. 2012. p. 159-179 https://doi.org/10.1017/CBO9781139004176.008
Galloway, Gregory J. / Constraints on the topology of higher-dimensional black holes. Black Holes in Higher Dimensions. Cambridge University Press, 2012. pp. 159-179
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