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Volumn 60, Issue 12, 1999, Pages

Effective action and thermodynamics of radiating shells in general relativity

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Indexed keywords


EID: 17044401239     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.124018     Document Type: Article
Times cited : (13)

References (35)
  • 24
    • 85037246420 scopus 로고    scopus 로고
    • J. Bicak (private communication).
    • Bicak, J.1
  • 25
    • 85037202438 scopus 로고    scopus 로고
    • The same approach is used in K. V. Kuchar, “Black hole formation by canonical dynamics of gravitating shells: an equatorial view,” report; and (private communication)
    • The same approach is used in K. V. Kuchar, “Black hole formation by canonical dynamics of gravitating shells: an equatorial view,” report; and (private communication).
  • 26
    • 85037225026 scopus 로고    scopus 로고
    • E. C. G. Sudarshan and N. Mukunda, Classical Dynamics: A modern perspective (Klieger, Malabur, FL, 1983)
    • E. C. G. Sudarshan and N. Mukunda, Classical Dynamics: A modern perspective (Klieger, Malabur, FL, 1983).
  • 30
    • 0001518757 scopus 로고
    • Indeed our results are analogous to those obtained for a black hole in a spherical cavity of radius R; see J.W. York, Phys. Rev. D 33, 2092 (1986).
    • (1986) Phys. Rev. D , vol.33 , pp. 2092
    • York, J.W.1
  • 31
    • 85037208037 scopus 로고    scopus 로고
    • We denote exact differentials by d and generic variations by (Formula presented)
    • We denote exact differentials by d and generic variations by (Formula presented).
  • 33
    • 85037242468 scopus 로고    scopus 로고
    • The general solution to Eq. (4.6) (having the units of a temperature) is given by a sum of powers of (Formula presented) and the fundamental constants of the form (Formula presented)and for (Formula presented) one obtains the temperature (4.7) one would expect a distance R from a black hole of mass (Formula presented)
    • The general solution to Eq. (4.6) (having the units of a temperature) is given by a sum of powers of (Formula presented) and the fundamental constants of the form (Formula presented)and for (Formula presented) one obtains the temperature (4.7) one would expect a distance R from a black hole of mass (Formula presented) 27.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.