Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime II. Quantum States and Hawking Radiation
arXiv:0805.0519 · doi:10.1103/PhysRevD.78.024019
Abstract
In a previous paper we studied the collapse of a spherically symmetric dust distribution (marginally bound LTB) in d-dimensional AdS spacetime and obtained the condition for the formation of trapped surfaces. Here we extend the analysis by giving the canonical theory for the same and subsequently quantize the system by solving the Wheeler-DeWitt equation. We show that for the case of small dust perturbations around a black hole the wave functionals so obtained describe an AdS-Schwarzschild black hole in equilibrium with a thermal bath at Hawking temperature and show the non-trivial dependence of this temperature on the number of spacetime dimensions and the cosmological constant.
20 pages
References in corpus (4)
- Hawking radiation from the quantum Lemaitre-Tolman-Bondi model
- Mass Spectrum and Statistical Entropy of the BTZ black hole from Canonical Quantum Gravity
- Quantum Gravitational Collapse and Hawking Radiation in 2+1 Dimensions
- Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime I. Classical Solutions