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8
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0033248454
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G. L. Alberghi, R. Casadio, G. P. Vacca, and G. Venturi, Class. Quantum Grav. 16, 131 (1999).
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(1999)
Class. Quantum Grav.
, vol.16
, pp. 131
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Alberghi, G.L.1
Casadio, R.2
Vacca, G.P.3
Venturi, G.4
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20
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0003713728
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Wiley, New York, L. Witten
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R. Arnowitt, S. Deser, and C. W. Misner, in Gravitation: An Introduction to Current Research, edited by L. Witten (Wiley, New York, 1962).
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(1962)
Gravitation: An Introduction to Current Research
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Arnowitt, R.1
Deser, S.2
Misner, C.W.3
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22
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0031521211
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S. Ansoldi, A. Aurilia, R. Balbinot, and E. Spallucci, Class. Quantum Grav. 14, 2727 (1997).
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(1997)
Class. Quantum Grav.
, vol.14
, pp. 2727
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Ansoldi, S.1
Aurilia, A.2
Balbinot, R.3
Spallucci, E.4
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24
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85037246420
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J. Bicak (private communication).
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Bicak, J.1
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25
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85037202438
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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)
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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).
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26
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85037225026
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E. C. G. Sudarshan and N. Mukunda, Classical Dynamics: A modern perspective (Klieger, Malabur, FL, 1983)
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E. C. G. Sudarshan and N. Mukunda, Classical Dynamics: A modern perspective (Klieger, Malabur, FL, 1983).
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30
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0001518757
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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).
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(1986)
Phys. Rev. D
, vol.33
, pp. 2092
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York, J.W.1
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31
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85037208037
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We denote exact differentials by d and generic variations by (Formula presented)
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We denote exact differentials by d and generic variations by (Formula presented).
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33
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85037242468
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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)
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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.
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