Evaporation of two-dimensional black holes

DOI10.1103/PhysRevLett.69.406zbMath0968.83512arXivhep-th/9203052OpenAlexW2055829555WikidataQ74519356 ScholiaQ74519356MaRDI QIDQ4491989

Stephen W. Hawking

Publication date: 16 July 2000

Published in: Physical Review Letters (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/9203052

Mathematics Subject Classification ID

Two-dimensional field theories, conformal field theories, etc. in quantum mechanics (81T40) Black holes (83C57)

Related Items (12)

Black hole thermodynamics. A classical non-equilibrium approach ⋮ On the initial value problem for semiclassical gravity without and with quantum state collapses ⋮ Quantum thermal effect of quasi-static evaporating charged black hole ⋮ Hawking’s radiation of sine–Gordon black holes in two dimensions ⋮ QUANTUM DILATONIC GRAVITY IN d=2,4 AND 5 DIMENSIONS ⋮ Classical and semiclassical properties of extremal black holes with dilaton and modulus fields. ⋮ Black hole evolution ⋮ Superstrings in 2D backgrounds with R-R flux and new extremal black holes ⋮ Sinh-Gordon matter field and a solvable model in two-dimensional gravity. ⋮ The classical solutions of two-dimensional gravity ⋮ DOES BLACK HOLE EVAPORATION IMPLY THAT PHYSICS IS NONUNITARY, AND IF SO, WHAT MUST THE LAWS OF PHYSICS LOOK LIKE? ⋮ Lineal gravity from planar gravity

Cites Work

• Particle creation by black holes
• Why there is nothing rather than something: A theory of the cosmological constant
• Wave function of the Universe

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