Semiclassical quantum states for black holes

DOI10.1016/S0920-5632(97)00365-4zbMath0976.83530arXivgr-qc/9701018OpenAlexW3123532401MaRDI QIDQ5927224

Claus Kiefer

Publication date: 8 March 2001

Published in: Nuclear Physics. B. Proceedings Supplements (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9701018

zbMATH Keywords

black hole entropyCGHS modeldecoherence of semiclassical statesHawking radiationsemiclassical approximationspherically symmetric gravityWheeler-De Witt equation

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45)

Related Items (1)

Ehrenfest's principle and the problem of time in quantum gravity

Cites Work

• Role of surface integrals in the Hamiltonian formulation of general relativity
• Why the Entropy of a Black Hole is<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">A</mml:mi><mml:mo>/</mml:mo><mml:mn>4</mml:mn><mml:mn /></mml:math>
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