Microfield dynamics of black holes

R. Casadio and B. Harms
Phys. Rev. D 58, 044014 – Published 22 July 1998
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Abstract

The microcanonical treatment of black holes as opposed to the canonical formulation is reviewed and some major differences are displayed. We propose a microcanonical alternative to the thermodynamical expression for the number density and discuss its characteristics. In particular the decay rates are compared in the two different pictures and shown to predict significantly different fates for cosmological black holes.

  • Received 12 December 1997

DOI:https://doi.org/10.1103/PhysRevD.58.044014

©1998 American Physical Society

Authors & Affiliations

R. Casadio* and B. Harms

  • Department of Physics and Astronomy, The University of Alabama, Tuscaloosa, Alabama 35487-0324

  • *Permanent address: Dipartimento di Fisica dell’Università di Bologna and I.N.F.N., Sezione di Bologna, via Irnerio 46, I-40126 Bologna, Italy.

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Vol. 58, Iss. 4 — 15 August 1998

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