Moving mirrors and event horizons in non-flat background geometry
From MaRDI portal
Publication:6573766
DOI10.1088/1361-6382/ad5bb4zbMATH Open1548.83072MaRDI QIDQ6573766
Publication date: 17 July 2024
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47) Analogues of general relativity in lower dimensions (83C80)
Cites Work
- Particle creation by black holes
- On horizonless temperature with an accelerating mirror
- Zoo of holographic moving mirrors
- Back-reaction in the moving mirror effects.
- Holographic models of de Sitter QFTs
- Quantum Field Theory in Curved Spacetime
- Radiation from a moving mirror in two dimensional space-time: conformal anomaly
- Black hole in three-dimensional spacetime
- Making anti-de Sitter black holes
- Particle production and positive energy theorems for charged black holes in DeSitter
- Geodesic structure of the (2 + 1)-dimensional BTZ black hole
- QUANTUM FIELDS IN SCHWARZSCHILD–DE SITTER SPACE
- Hawking radiation particle spectrum of a Kerr-Newman black hole
- Upon the horizon’s verge: Thermal particle creation between and approaching horizons
- Accelerating boundary analog of a Kerr black hole
- On the duality of Schwarzschild–de Sitter spacetime and moving mirror
- Quantum Fields in Curved Space
This page was built for publication: Moving mirrors and event horizons in non-flat background geometry
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6573766)
