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Volumn 64, Issue 12, 2001, Pages

Asymptotic symmetries on killing horizons

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; ENTROPY; GRAVITY; MATHEMATICS; ROTATION; THEORY;

EID: 85038286456     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (110)

References (47)
  • 1
    • 0041686993 scopus 로고    scopus 로고
    • see, for review, G.T. Horowitz, gr-qc/9604051
    • A. Strominger and C. Vafa, Phys. Lett. B 379, 99 (1996); see, for review, G.T. Horowitz, gr-qc/9604051.
    • (1996) Phys. Lett. B , vol.379 , pp. 99
    • Strominger, A.1    Vafa, C.2
  • 17
    • 0000137796 scopus 로고
    • Phys. Rev. 128, 2851 (1962).
    • (1962) Phys. Rev. , vol.128 , pp. 2851
  • 31
    • 33750556099 scopus 로고    scopus 로고
    • note
    • In general, the hypersurface orthogonality holds only on the horizon. However, in the case of static and spherically symmetric spacetimes, it is globally valid.
  • 32
    • 85107715213 scopus 로고    scopus 로고
    • note
    • μν are analytic without loss of generality, because higher-order terms in υ do not make any contribution.
  • 33
    • 85107715434 scopus 로고    scopus 로고
    • note
    • (h)β)/2 give the same value of the surface gravity as that defined by Eq. (2.9). These definitions of the surface gravity result from Eq. (2.9), by using Eqs. (2.6) and (2.8).
  • 35
    • 33750539665 scopus 로고    scopus 로고
    • note
    • In the Euclidean approach to black hole thermodynamics [25], the temperature of a black hole is derived by imposing regular periodicity near the horizon in the Euclidean section. However, in this case also, we will need to specify the global behavior of the Euclidean section, so that the system is in thermal equilibrium, i.e., the Hartle-Hawking state. In fact, the energy-momentum tensor is singular on the horizon when we consider a quantum field out of equilibrium in a static spacetime [26].
  • 37
    • 0004048969 scopus 로고
    • edited by S. Hawking and W. Israel Cambridge University Press, Cambridge, England
    • S. Hawking, in General Relativity, edited by S. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1979).
    • (1979) General Relativity
    • Hawking, S.1
  • 39
    • 33750565970 scopus 로고    scopus 로고
    • note
    • The Euclidean approach to black hole thermodynamics played a crucial role in choosing a specific form of the symmetry vectors in Refs. [11,12].
  • 40
    • 85107712448 scopus 로고    scopus 로고
    • note
    • βα(g;ζ) in Eq. (4.20) are defined only up to ambiguity [17]. Here, we make a natural choice, and the effects of the ambiguity will be discussed in future investigations.
  • 41
    • 85107712130 scopus 로고    scopus 로고
    • note
    • ζ2 in Ref. [12].
  • 45
    • 33750547926 scopus 로고    scopus 로고
    • A. Strominger, hep-th/0106113
    • A. Strominger, hep-th/0106113.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.