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Thermal statistical ensembles of black holes

Author

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  • Chevalier, C.
  • Bustamante, M.
  • Debbasch, F.

Abstract

We consider statistical ensembles of Schwarzschild black holes and prove that these ensembles describe black holes of nonvanishing temperatures. The mean space–times associated to these ensembles are explored through exact computations of their energy distributions, total masses and calorific capacities. We discuss our results, with special emphasis on their connections with current and near future observations of astrophysical black holes, string theory and cosmology.

Suggested Citation

  • Chevalier, C. & Bustamante, M. & Debbasch, F., 2007. "Thermal statistical ensembles of black holes," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 376(C), pages 293-307.
    • Handle: RePEc:eee:phsmap:v:376:y:2007:i:c:p:293-307
    DOI: 10.1016/j.physa.2006.10.062
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    References listed on IDEAS

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    1. F. Debbasch, 2004. "What is a mean gravitational field?," The European Physical Journal B: Condensed Matter and Complex Systems, Springer;EDP Sciences, vol. 37(2), pages 257-269, January.
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    Cited by:

    1. Chevalier, Claire & Debbasch, Fabrice & Ollivier, Yann, 2009. "Multiscale cosmological dynamics," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 388(24), pages 5029-5035.

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    1. Chevalier, Claire & Debbasch, Fabrice & Ollivier, Yann, 2009. "Multiscale cosmological dynamics," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 388(24), pages 5029-5035.
    2. Chevalier, C. & Debbasch, F., 2009. "Thermal statistical ensembles of classical extreme black holes," Physica A: Statistical Mechanics and its Applications, Elsevier, vol. 388(5), pages 628-638.

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