On time evolution of quantum black holes

DOI10.1016/S0370-2693(01)00634-7zbMath0969.83513arXivgr-qc/0102006OpenAlexW3099837725MaRDI QIDQ5936303

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Publication date: 10 July 2001

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0102006

zbMATH Keywords

semiclassical approximationcanonical quantum gravity equationsHamiltonian constraint

Mathematics Subject Classification ID

Black holes (83C57) Quantization of the gravitational field (83C45)

Related Items (4)

Quantum rotating black holes ⋮ Bohmian trajectories for an evaporating blackhole ⋮ Dilaton gravity in two dimensions ⋮ A quantum state for the late universe

Cites Work

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• What simplified models say about unitarity and gravitational collapse
• Particle creation by black holes
• ON THE DYNAMICS OF SPHERICALLY SYMMETRIC SYSTEMS IN QUANTUM GRAVITY
• The Born - Oppenheimer approach to the matter - gravity system and unitarity
• Exact Quantization Conditions. II
• Quantum Theory of Gravity. I. The Canonical Theory
• Quantum Fields in Curved Space

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