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  Quasi-local rotating black holes in higher dimension: geometry

Lewandowski, J., & Pawlowski, T. (2005). Quasi-local rotating black holes in higher dimension: geometry. Classical and Quantum Gravity, 22(9), 1573-1598.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-4E26-7 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-4E27-5
Genre: Journal Article

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cqg5_9_007.pdf (Publisher version), 264KB
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 Creators:
Lewandowski, Jerzy1, Author
Pawlowski, Tomasz1, Author
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1Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24014              

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 Abstract: With the help of a generalized Raychaudhuri equation non-expanding null surfaces are studied in an arbitrary dimensional case. The definition and basic properties of non-expanding and isolated horizons known in the literature in the four- and three-dimensional cases are generalized. A local description of the horizon's geometry is provided. The zeroth law of black-hole thermodynamics is derived. The constraints have a similar structure to that of the four-dimensional spacetime case. The geometry of a vacuum isolated horizon is determined by the induced metric and the rotation 1-form potential, local generalizations of the area and the angular momentum typically used in the stationary black-hole solutions case.

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Language(s): eng - English
 Dates: 2005-05-07
 Publication Status: Issued
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 Identifiers: eDoc: 251036
ISI: 000229354400010
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Title: Classical and Quantum Gravity
  Alternative Title : Class. Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 22 (9) Sequence Number: - Start / End Page: 1573 - 1598 Identifier: ISSN: 0264-9381