Tunneling during Quantum Collapse in AdS Spacetime
arXiv:1204.5466 · doi:10.1103/PhysRevD.87.024045
Abstract
We extend previous results on the reflection and transmission of self-gravitating dust shells across the apparent horizon during quantum dust collapse to non-marginally-bound dust collapse in arbitrary dimensions with a negative cosmological constant. We show that the Hawking temperature is independent of the energy function and that the wave functional describing the collapse is well behaved at the Hawking-Page transition point. Thermal radiation from the apparent horizon appears as a generic result of non-marginal collapse in AdS space-time owing to the singular structure of the Hamiltonian constraint at the apparent horizon.
14 pages. No figures. Title changed to published version
References in corpus (6)
- Hawking radiation from the quantum Lemaitre-Tolman-Bondi model
- Quantum Gravitational Collapse and Hawking Radiation in 2+1 Dimensions
- Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime I. Classical Solutions
- Spectrum and Statistical Entropy of AdS Black Holes
- Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime II. Quantum States and Hawking Radiation
- Reflection and Transmission at the Apparent Horizon during Gravitational Collapse