A Note on the Generalization of the GEMS Approach
arXiv:gr-qc/0410077 · doi:10.1103/PhysRevD.71.104008
Abstract
This paper is a supplement of our earlier work JHEP 0410 (2004) 011[gr-qc/0409107].We map the vector potential of charged black holes into GEMS and find that its effect on the thermal spectrum is the same as that on the black hole side, i.e., it will induce a chemical potential in the thermal spectrum which is the same as that in the charged black holes.We also argue that the generalization of GEMS approach to non-stationary motions is not possible.
Latex file, 10 pages, no figure; v2: minor corrections; v3: revised with title changed, one new section added and references added
References in corpus (5)
- Accelerated Detectors and Temperature in (Anti) de Sitter Spaces
- Mapping Hawking into Unruh Thermal Properties
- Equivalence of Hawking and Unruh Temperatures and Entropies Through Flat Space Embeddings
- The GEMS Approach to Stationary Motions in the Spherically Symmetric Spacetimes
- Complete higher dimensional global embedding structures of various black holes
Cited by in corpus (9)
- Causal particle detectors and topology
- A New Global Embedding Approach to Study Hawking and Unruh Effects
- Accelerating Branes and Brane Temperature
- Relativistic Kinematics and Stationary Motions
- De Sitter Thermodynamics from Diamonds's Temperature
- Global Embedding of the Reissner-Nordström Metric in the Flat Ambient Space
- What Hawking Radiation Looks Like as You Fall into a Black Hole
- Accelerated paths and Unruh effect I: scalars and fermions in Anti De Sitter spacetime
- Mapping Hawking temperature in the spinning constant curvature black hole spaces into Unruh temperature