Black Hole - Moving Mirror I: An Exact Correspondence
arXiv:1507.03489 · doi:10.1142/9789813226609_0171
Abstract
An exact correspondence is shown between a new moving mirror trajectory in (1+1)D and a spacetime in (1+1)D in which a black hole forms from the collapse of a null shell. It is shown that the Bogolubov coefficients between the "in" and "out" states are identical and the exact Bogolubov coefficients are displayed. Generalization to the (3+1)D black hole case is discussed.
Contribution to MG14 Proceedings, 5 pages, 1 figure
Cited by in corpus (12)
- Remnant-free Moving Mirror Model for Black Hole Radiation Field
- Entanglement Harvesting with Moving Mirrors
- Extreme Hawking Radiation
- The mirror at the edge of the universe: Reflections on an accelerated boundary correspondence with de Sitter cosmology
- Finite Energy but Infinite Entropy Production from Moving Mirrors
- Particle spectrum of the Reissner-Nordström black hole
- Spacetime continuity and quantum information loss
- Accelerating boundary analog of a Kerr black hole
- Observational signature of Lorentz violation in acceleration radiation
- Schwarzschild Metric with Planck Length
- Analog Particle Production Model for General Classes of Taub-NUT Black Holes
- Quantum aspects of spacetime: A quantum optics view of acceleration radiation and black holes