Information preservation for null shell collapse: a moving mirror model
DOI10.1007/S10714-019-2575-5zbMath1429.83045arXiv1801.08020OpenAlexW3101987461MaRDI QIDQ2272557
Publication date: 10 September 2019
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1801.08020
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Space-time singularities, cosmic censorship, etc. (83C75) Measures of information, entropy (94A17) Quantum information, communication, networks (quantum-theoretic aspects) (81P45)
Related Items (5)
Cites Work
- Last gasp of a black hole: unitary evaporation implies non-monotonic mass loss
- Particle creation by black holes
- Black holes are one-dimensional
- On horizonless temperature with an accelerating mirror
- Transition to light-like trajectories in thin shell dynamics
- Boundary dynamics in gravitational theories
- Signatures of energy flux in particle production: a black hole birth cry and death gasp
- Radiation from a moving mirror in two dimensional space-time: conformal anomaly
This page was built for publication: Information preservation for null shell collapse: a moving mirror model