Thermal Wightman Functions and Renormalized Stress Tensors in the Rindler Wedge
arXiv:hep-th/9507139 · doi:10.1016/0370-2693(96)00223-7
Abstract
The Wightman functions in the Rindler portion of Minkowski space-time are presented for any value of the temperature and for massless spin fields up to s=1 and the renormalized stress tensor relative to Minkowski vacuum is discussed. A gauge ambiguity in the vector case is pointed out.
arXiv commentMore comments and formulas added in the case of spin 1, a few signs changed in some formulas, it will appear on Phys. Lett
References in corpus (2)
Cited by in corpus (19)
- Electromagnetic fields in Schwarzschild and Reissner-Nordström geometry. Quantum corrections to the black hole entropy
- Direct -function approach and renormalization of one-loop stress tensors in curved spacetimes
- The Casimir effect in the Fulling-Rindler vacuum
- Entanglement and Thermal Entropy of Gauge Fields
- Noise kernels of stochastic gravity in conformally-flat spacetimes
- Canonical Quantization of Photons in a Rindler Wedge
- Varying the Unruh Temperature in Integrable Quantum Field Theories
- Fermionic condensate and the mean energy-momentum tensor in the Fulling-Rindler vacuum
- Exploring the Rindler vacuum and the Euclidean Plane
- Geometric Entropy and Curvature Coupling in Conical Spaces: zeta Function Approach
- A relationship between scalar Green functions on hyperbolic and Euclidean Rindler spaces
- A Bisognano-Wichmann-like Theorem in a Certain Case of a Non Bifurcate Event Horizon related to an Extreme Reissner-Nordström Black Hole
- Localized thermal states and negative energy
- Vacuum Quantum Effects for Parallel Plates Moving by Uniform Acceleration in Static de Sitter Space
- Thermal fluctuations of a quantized massive scalar field in Rindler background
- Remarks on Rindler Quantization
- Quantum Energy Inequalities along stationary worldlines
- Euclidean Thermal Green Functions of Photons in Generalized Euclidean Rindler Spaces for any Feynman-like Gauge
- Fermionic Casimir densities for a uniformly accelerating mirror in the Fulling-Rindler vacuum