1997Unpublished venueRequires access

SEMICLASSICAL QUANTUM STATES FOR BLACK HOLES 1

Claus Kiefer

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Abstract

I discuss the semiclassical approximation for the Wheeler–DeWitt equation when applied to the CGHS model and spherically symmetric gravity. Special attention is devoted to the issues of Hawking radiation, decoherence of semiclassical states, and black hole entropy. 1 Dedicated to Tullio Regge on his sixty–fifth birthday. To appear in the Proceedings

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What this paper is about

I discuss the semiclassical approximation for the Wheeler–DeWitt equation when applied to the CGHS model and spherically symmetric gravity. Special attention is devoted to the issues of Hawking radiation, decoherence of semiclassical states, and black hole entropy. 1 Dedicated to Tullio Regge on his sixty–fifth birthday. To appear in the Proceedings

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Available abstract

I discuss the semiclassical approximation for the Wheeler–DeWitt equation when applied to the CGHS model and spherically symmetric gravity. Special attention is devoted to the issues of Hawking radiation, decoherence of semiclassical states, and black hole entropy. 1 Dedicated to Tullio Regge on his sixty–fifth birthday. To appear in the Proceedings

Key concepts: Semiclassical physics, Hawking radiation, Physics, Semiclassical gravity, Quantum decoherence, Black hole (networking), Quantum gravity, Black hole information paradox

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