Black-Hole Thermodynamics, Mass-Inflation, and Evaporation View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1992

AUTHORS

Don N. Page

ABSTRACT

The negative specific heat of black holes in asymptotically flat spacetime gives rise to unusual thermal properties, such as the nonexistence of the canonical ensemble (though it would exist if there were a negative cosmological constant or if the local temperature at the surface of a box were somehow kept fixed). A black hole can dominate the microcanonical ensemble in an impervious box with energy greater than a calculable multiple of the volume to the one-fifth power. The rate at which ordinary thermal radiation would go to such a black-hole configuration is estimated and various self-gravity corrections are calculated. A homogeneous model for mass inflation inside a spherical charged black hole with equal amounts of ingoing and outgoing radial null radiation is considered. In this overly simplified model, the singularity is shown to be spacelike rather than null. Some thoughts are presented on Planck’s form of the third law for black hole thermodynamics, and on the possible degree of quantum unpredictability there may be in black-hole formation and evaporation. More... »

PAGES

185-224

References to SciGraph publications

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  • 1985-11. Self-gravitating radiation in anti-de sitter space in GENERAL RELATIVITY AND GRAVITATION
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  • 1981-12. Entropy of self-gravitating radiation in GENERAL RELATIVITY AND GRAVITATION
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  • Book

    TITLE

    Black Hole Physics

    ISBN

    978-94-010-5067-8
    978-94-011-2420-1

    Author Affiliations

    Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/978-94-011-2420-1_5

    DOI

    http://dx.doi.org/10.1007/978-94-011-2420-1_5

    DIMENSIONS

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