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How red is a quantum black hole?

Husain, Viqar and Winkler, Oliver (2005) How red is a quantum black hole? [Preprint]

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    Abstract

    Radiating black holes pose a number of puzzles for semiclassical and quantum gravity. These include the transplanckian problem – the nearly infinite energies of Hawking particles created near the horizon, and the final state of evaporation. A definitive resolution of these questions likely requires robust inputs from quantum gravity. We argue that one such input is a quantum bound on curvature. We show how this leads to an upper limit on the redshift of a Hawking emitted particle, to a maximum temperature for a black hole, and to the prediction of a Planck scale remnant.

    Item Type: Preprint
    Additional Information: pubdom TRUE
    Uncontrolled Keywords: AARMS
    Subjects: 84-xx Astronomy and astrophysics
    Faculty: UNSPECIFIED
    Depositing User: lingyun ye
    Date Deposited: 09 Jul 2007
    Last Modified: 27 Apr 2010 16:36
    URI: https://docserver.carma.newcastle.edu.au/id/eprint/358

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