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2
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2442464088
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in General Relativity An Einstein Century Survey, edited by S.W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1979), p. 581.
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R. Penrosereprinted in Gen. Relativ. Gravit. 34, 1141 (2002);in General Relativity, An Einstein Century Survey, edited by S.W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1979), p. 581.
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Gen. Relativ. Gravit.
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Penrose, R.1
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6
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0032476525
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S. Barve, T.P. Singh, C. Vaz, and L. Witten, Nucl. Phys. B532, 361 (1998)
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(1998)
Nucl. Phys.
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Barve, S.1
Singh, T.P.2
Vaz, C.3
Witten, L.4
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21
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85039602862
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B.J. Carr, in Proceedings of the Ninth Workshop on General Relativity and Gravitation, Hiroshima, Japan, 1999, edited by Y. Eriguchi et al., p. 425, gr-qc/0003009.
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Carr, B.J.1
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25
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85039591677
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One can prove (Formula presented) with the dominant energy condition on collapsing matter, and the equality is excluded by a physically reasonable requirement on the collapsing matter at the CH 20
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One can prove (Formula presented) with the dominant energy condition on collapsing matter, and the equality is excluded by a physically reasonable requirement on the collapsing matter at the CH 20.
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26
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85039596756
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The time (Formula presented) can be regarded as the Planck time (Formula presented) at least this is the case for the self-similar dust model.
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The time (Formula presented) can be regarded as the Planck time (Formula presented) at least this is the case for the self-similar dust model.
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27
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85037874162
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T. Harada, H. Iguchi, K. Nakao, T. Tanaka, T.P. Singh, and C. Vaz, Phys. Rev. D 64, 041501 (2001).
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(2001)
Phys. Rev. D
, vol.64
, pp. 41501
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Harada, T.1
Iguchi, H.2
Nakao, K.3
Tanaka, T.4
Singh, T.P.5
Vaz, C.6
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28
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85039590845
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When the CH and event horizon exactly coincide, the radiation is reduced to the Hawking radiation 3 4. This fact cannot be derived with the method making use of the local map since in this case (Formula presented) in Eq. (3.1). This is not surprising, since an event horizon, which plays a central role in the Hawking radiation, is not a local object but a global one.
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When the CH and event horizon exactly coincide, the radiation is reduced to the Hawking radiation 34. This fact cannot be derived with the method making use of the local map since in this case (Formula presented) in Eq. (3.1). This is not surprising, since an event horizon, which plays a central role in the Hawking radiation, is not a local object but a global one.
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37
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85039595600
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U. Miyamoto and T. Harada (in preparation).
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U. Miyamoto and T. Harada (in preparation).
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