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  The spacetime in the neighborhood of a general isolated black hole

Krishnan, B. (2012). The spacetime in the neighborhood of a general isolated black hole. Classical and quantum gravity, 29(20): 205006. doi:10.1088/0264-9381/29/20/205006.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000E-E9AB-8 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000E-E9AC-6
Genre: Journal Article

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1204.4345 (Preprint), 469KB
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 Creators:
Krishnan, Badri1, Author              
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: We construct the spacetime in the vicinity of a general isolated, rotating, charged black hole. The black hole is modeled as a weakly isolated horizon, and we use the characteristic initial value formulation of the Einstein equations with the horizon as an inner boundary. The spacetime metric and other geometric fields are expanded in a power series in a radial coordinate away from the horizon by solving the characteristic field equations in the Newman-Penrose formalism. This is the first in a series of papers which investigate the near horizon geometry and its physical applications using the isolated horizon framework.

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 Dates: 2012-04-192012
 Publication Status: Published in print
 Pages: 23 pages, 1 figure
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1204.4345
DOI: 10.1088/0264-9381/29/20/205006
 Degree: -

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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 29 (20) Sequence Number: 205006 Start / End Page: - Identifier: ISSN: 0264-9381
CoNE: /journals/resource/954925513480_1