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4
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85038997336
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see, for a review, G. T. Horowitz, gr-qc/9604051.
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Horowitz, G.T.1
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6
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33750667450
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8
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21144459871
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The zeroth law is proved for an arbitrary static or stationary axisymmetric black hole spacetime in CQGRDG
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I. Racz and R. M. Wald, Class. Quantum Grav. 9, 2643 (1992). The zeroth law is proved for an arbitrary static or stationary axisymmetric black hole spacetime in CQGRDG
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Wald, R.M.2
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10
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23544457811
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Wald, R.M.1
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19
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0001476008
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PYLBAJ
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4243758900
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Futamase, T.1
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24
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85039012908
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We adopt the tensor component notation for simplicity of expressions, instead of the abstract index notation used in R. M. Wald, General Relativity (University of Chicago Press, Chicago, 1984).
-
We adopt the tensor component notation for simplicity of expressions, instead of the abstract index notation used in R. M. Wald, General Relativity (University of Chicago Press, Chicago, 1984).
-
-
-
-
25
-
-
85038977615
-
-
The matrix (Formula presented) is regarded as a 10×10 matrix, whose elements are given by the second derivative of (Formula presented) by the independent components of (Formula presented) 21
-
The matrix (Formula presented) is regarded as a 10×10 matrix, whose elements are given by the second derivative of (Formula presented) by the independent components of (Formula presented) 21.
-
-
-
-
26
-
-
85039007764
-
-
The thermodynamical variables do not change even if we include the totally divergent term in the case of stationary black holes. However, it results in ambiguity of the definition of the entropy in dynamical processes 9
-
The thermodynamical variables do not change even if we include the totally divergent term in the case of stationary black holes. However, it results in ambiguity of the definition of the entropy in dynamical processes 9.
-
-
-
-
28
-
-
85038982550
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-
The essential part of this subsection has been already noted in Ref. 11
-
The essential part of this subsection has been already noted in Ref. 11.
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35
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0000852959
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36
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0000637732
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PRVDAQ
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G. Kang, Phys. Rev. D 54, 7483 (1996). PRVDAQ
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Kang, G.1
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