Mapping Hawking into Unruh thermal properties
- 1 February 1999
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 59 (6) , 064004
- https://doi.org/10.1103/physrevd.59.064004
Abstract
By globally embedding curved spaces into higher dimensional flat ones, we show that Hawking thermal properties map into their Unruh equivalents: The relevant curved space detectors become Rindler ones, whose temperature and entropy reproduce the originals. Specific illustrations include Schwarzschild, Schwarzschild–(anti-)de Sitter, Reissner-Nordström, and Bañados-Teitelboim-Zanelli spaces.Keywords
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This publication has 19 references indexed in Scilit:
- Equivalence of Hawking and Unruh temperatures and entropies through flat space embeddingsClassical and Quantum Gravity, 1998
- Accelerated detectors and temperature in (anti-) de Sitter spacesClassical and Quantum Gravity, 1997
- HOW HOT IS THE DE SITTER SPACE?International Journal of Modern Physics B, 1996
- The (2 + 1)-dimensional black holeClassical and Quantum Gravity, 1995
- Temperature, energy, and heat capacity of asymptotically anti–de Sitter black holesPhysical Review D, 1994
- Geometry of the 2+1 black holePhysical Review D, 1993
- Black hole in three-dimensional spacetimePhysical Review Letters, 1992
- Entropy of a Rindler wedgePhysics Letters B, 1987
- Particle creation by black holesCommunications in Mathematical Physics, 1975
- Black Holes and EntropyPhysical Review D, 1973