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Volumn 69, Issue 10, 2004, Pages

Semiclassical instability of the Cauchy horizon in self-similar collapse

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[No Author keywords available]

Indexed keywords


EID: 3042699897     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.104005     Document Type: Article
Times cited : (9)

References (37)
  • 2
    • 2442464088 scopus 로고    scopus 로고
    • in General Relativity An Einstein Century Survey, edited by S.W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1979), p. 581.
    • 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.
    • (2002) Gen. Relativ. Gravit. , vol.34 , pp. 1141
    • Penrose, R.1
  • 21
    • 85039602862 scopus 로고    scopus 로고
    • 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.
    • Carr, B.J.1
  • 25
    • 85039591677 scopus 로고    scopus 로고
    • 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
    • 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.
  • 26
    • 85039596756 scopus 로고    scopus 로고
    • 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.
    • 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.
  • 28
    • 85039590845 scopus 로고    scopus 로고
    • 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.
    • 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.
  • 37
    • 85039595600 scopus 로고    scopus 로고
    • U. Miyamoto and T. Harada (in preparation).
    • U. Miyamoto and T. Harada (in preparation).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.