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Physical Review D

Volumn 52, Issue 8, 1995, Pages 4430-4439

Comparison of the Noether charge and Euclidean methods for computing the entropy of stationary black holes

(2) Iyer, Vivek a Wald, Robert M a

a UNIVERSITY OF CHICAGO (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 4243563509 PISSN: 05562821 EISSN: None Source Type: Journal
DOI: 10.1103/PhysRevD.52.4430 Document Type: Article

Times cited : (432)

References (19)

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- Matter fields ψ can be included straightforwardly if Lv ψ = 0 on Σt for all va, which vanish on Σt. For higher derivative gravity theories, one undoubtedly would need to generalize the choice of X boundary conditions given in assumption (1) to include the appropriate additional ``configuration" degrees of freedom associated with the spacetime metric.

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.