Quantum fields during black hole formation: how good an approximation is the Unruh state?
DOI10.1007/JHEP05(2018)140zbMath1391.83079arXiv1804.01228OpenAlexW2795758427WikidataQ129782051 ScholiaQ129782051MaRDI QIDQ1651168
Benito A. Juárez-Aubry, Jorma Louko
Publication date: 11 July 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1804.01228
Black holes (83C57) Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Analogues of general relativity in lower dimensions (83C80)
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- On the construction of Hartle-Hawking-Israel states across a static bifurcate Killing horizon
- Particle creation by black holes
- Theorems on the uniqueness and thermal properties of stationary, nonsingular, quasifree states on spacetimes with a bifurcate Killing horizon
- Rigorous construction and Hadamard property of the Unruh state in Schwarzschild spacetime
- The generally covariant locality principle -- a new paradigm for local quantum field theory
- Quantum energy inequalities and local covariance. II: Categorical formulation
- On smooth Cauchy hypersurfaces and Geroch's splitting theorem
- Smoothness of time functions and the metric splitting of globally hyperbolic spacetimes
- Algebraic QFT in Curved Spacetime and Quasifree Hadamard States: An Introduction
- QUANTUM FIELD THEORY ON CURVED BACKGROUNDS — A PRIMER
- Onset and decay of the 1 + 1 Hawking–Unruh effect: what the derivative-coupling detector saw
- Phenomenological description of the interior of the Schwarzschild black hole
- Quantum energy inequalities and local covariance. I. Globally hyperbolic spacetimes
- Radiation from a moving mirror in two dimensional space-time: conformal anomaly
- A SELF-CONSISTENT MODEL OF THE BLACK HOLE EVAPORATION
- A linear approximation to black hole evaporation
- Quantum Fields in Curved Space
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