Notes on peculiarities of quantum fields in space–times with horizons

DOI10.1088/1361-6382/AC8F0EOpenAlexW4226073666MaRDI QIDQ5869425

K. V. Bazarov

Publication date: 28 September 2022

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2112.02188

zbMATH Keywords

Hawking radiationde Sitter spaceSchwarzschild black holeRindler spaceUnruh effectquantum fields in curved space-times

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20) Methods of quantum field theory in general relativity and gravitational theory (83C47) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Observers (93B53)

Related Items (2)

TCC bounds on the static patch of de Sitter space ⋮ Quantization of spinor field in the Schwarzschild spacetime and spin sums for solutions of the Dirac equation

Cites Work

• Unnamed Item
• Particle creation by black holes
• Theorems on the uniqueness and thermal properties of stationary, nonsingular, quasifree states on spacetimes with a bifurcate Killing horizon
• On the orthogonality of the MacDonald's functions
• On the near-horizon geometry of an evaporating black hole
• Quantum field theory in the de sitter universe
• Curved space equilibration versus flat space thermalization: A short review
• LECTURE NOTES ON INTERACTING QUANTUM FIELDS IN DE SITTER SPACE
• Quantum Fields in Curved Space

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