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Cited by 215

The DOI matches its Crossref record; 7 of the 7 references it cites were found in a registry or an index.

Mechanics of isolated horizons

Open access
Ashtekar, Abhay, Beetle, Christopher, Fairhurst, Stephen·2000·Classical and Quantum Gravity

Abstract

A set of boundary conditions defining an undistorted, non-rotating isolated horizon are specified in general relativity. A spacetime representing a black hole which is itself in equilibrium but whose exterior contains radiation admits such a horizon. However, the definition is applicable in a more general context, such as cosmological horizons. Physically motivated, (quasi-)local definitions of the mass and surface gravity of an isolated horizon are introduced and their properties analysed. Although their definitions do not refer to infinity, these quantities assume their standard values in the static black-hole solutions. Finally, using these definitions, the zeroth and first laws of black-hole mechanics are established for isolated horizons.

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Crossref · 10.1088/0264-9381/17/2/301

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Metadata

Authors
Ashtekar, A., Beetle, C., & Fairhurst, S.
Venue
Classical and Quantum Gravity
Published
1999-12-21
Volume
17
Issue
2
Pages
253-298
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2003566906
Cited by
215
References
7
FWCI
9.00
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Mechanics of isolated horizons. https://app.cochat.ai/papers/10.1088/0264-9381/17/2/301
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Ashtekar, A., Beetle, C., & Fairhurst, S. (2000). Mechanics of isolated horizons. Classical and Quantum Gravity. https://doi.org/10.1088/0264-9381/17/2/301

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.