The GEMS Approach to Stationary Motions in the Spherically Symmetric Spacetimes
arXiv:gr-qc/0409107 · doi:10.1088/1126-6708/2004/10/011
Abstract
We generalize the work of Deser and Levin on the unified description of Hawking radiation and Unruh effect to general stationary motions in spherically symmetric black holes. We have also matched the chemical potential term of the thermal spectrum of the two sides for uncharged black holes.
Latex file, 12 pages, no figure; v2: typos fixed; v3: minor corrections, final version published in JHEP
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Cited by in corpus (16)
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- Temperature versus acceleration: the Unruh effect for holographic models
- Accelerating Branes and Brane Temperature
- Hawking into Unruh mapping for embeddings of hyperbolic type
- Corrections to Unruh effect in tunneling formalism and mapping with Hawking effect
- Local free-fall Temperature of GMGHS Black Holes
- De Sitter Thermodynamics from Diamonds's Temperature
- A Note on the Generalization of the GEMS Approach
- When does the Hawking into Unruh mapping for global embeddings work?
- Local free-fall temperatures of charged BTZ black holes in massive gravity
- Local free-fall Temperature of modified Schwarzschild black hole in rainbow spacetime
- What Hawking Radiation Looks Like as You Fall into a Black Hole
- GEMS embeddings of Schwarzschild and RN black holes in Painlevé-Gullstrand spacetimes
- Embedding into flat spacetime and black hole thermodynamics
- Relation between quantum effects in General Relativity and embedding theory
- GEMS embeddings of Hayward regular black holes in massless and massive gravities