Abstract
Equilibrium configurations of self-gravitating massless thermal radiation inside spherical boxes of radiusR in asymptotically anti-de Sitter space (A = -3/b 2) are constructed numerically for a range of central densities. For each box radius considered (R/b = 0, 1/2, 1, 2, 4, ∞), there is a unique configuration with maximal total mass and entropy, and another (at a lower central density) with maximum asymptotic red-shifted temperature. With the box removed toR=∞, the maximum total mass and entropy of self-gravitating thermal radiation areM max≈ 0.4598b≈0.7964(−A)−1/2 andS max≈1.3560a 1/4 b 3/2≈ 3.0910a 1/4(−A)−3/4, and the maximum red-shifted temperature is
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References
Antonov, V. A. (1962).Vestnik Leningrad. Gos. Univ.,7, 135.
Lynden-Bell, D., and Wood, R. (1968).Mon. Not. R. Astron. Soc.,138, 495–525.
Bekenstein, J. D. (1973).Phys. Rev. D,7, 2333–2346.
Hawking, S. W. (1975).Commun. Math. Phys.,43, 199–220.
Sorkin, R., Wald, R. M., and Zhang, Z. J. (1981).Gen. Rel. Grav.,13, 1127–1146.
Hawking, S. W., and Page, D. N. (1983).Commun. Math. Phys.,87, 577–588.
Hawking, S. W. (1976).Phys. Rev. D,13, 191–197.
Hawking, S. W., and Ellis, G. F. R. (1973).The Large-Scale Structure of Space-Time (Cambridge University Press, Cambridge).
Chandrasekhar, S. (1972). InGeneral Relativity: Papers in Honour of J. L. Synge, L. O'Raifeartaigh, ed. (Clarendon Press, Oxford).
IMSL Inc. (1983).Reference Manual (Houston, Texas).
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Page, D.N., Phillips, K.C. Self-gravitating radiation in anti-de sitter space. Gen Relat Gravit 17, 1029–1042 (1985). https://doi.org/10.1007/BF00774206
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DOI: https://doi.org/10.1007/BF00774206