Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime II. Quantum States and Hawking Radiation

dc.creatorVaz, Cenalo
dc.creatorTibrewala, Rakesh
dc.creatorSingh, T. P.
dc.date2008-05-05
dc.date.accessioned2026-07-07T11:50:33Z
dc.date.available2026-07-07T11:50:33Z
dc.descriptionIn 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.
dc.description20 pages
dc.identifierhttps://arxiv.org/abs/0805.0519
dc.identifierhttp://arxiv.org/abs/0805.0519
dc.identifierPhys.Rev.D78:024019,2008
dc.identifierdoi:10.1103/PhysRevD.78.024019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203595
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleClassical and Quantum Gravitational Collapse in d-dim AdS Spacetime II. Quantum States and Hawking Radiation
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