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Thermal statistical ensembles of classical extreme black holes

Author

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  • Chevalier, C.
  • Debbasch, F.

Abstract

New statistical ensembles of classical extreme black holes are introduced. Each ensemble is proven to represent a non extreme, finite temperature black hole. This mean or average black hole is surrounded by a mean electromagnetic field and a so-called apparent matter, which is the large scale trace of the averaged upon small scale fluctuations of the gravitational and electromagnetic fields. However, the total mass and the total charge of space–time is not modified by the averaging.

Suggested Citation

  • 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.
    • Handle: RePEc:eee:phsmap:v:388:y:2009:i:5:p:628-638
    DOI: 10.1016/j.physa.2008.10.040
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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. & 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.

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