Classical and Quantum Gravitational Collapse in d-dim AdS Spacetime I. Classical Solutions

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dc.creatorTibrewala, Rakesh
dc.creatorGutti, Sashideep
dc.creatorSingh, T. P.
dc.creatorVaz, Cenalo
dc.date2007-12-10
dc.date2008-02-06
dc.date.accessioned2026-07-07T11:39:17Z
dc.date.available2026-07-07T11:39:17Z
dc.descriptionWe study the collapse of a spherically symmetric dust distribution in $d$-dimensional AdS spacetime. We investigate the role of dimensionality, and the presence of a negative cosmological constant, in determining the formation of trapped surfaces and the end state of gravitational collapse. We obtain the self-similar solution for the case of zero cosmological constant, and show that one cannot construct a self-similar solution when a cosmological constant is included.
dc.description19 pages, sections on surface gravity removed, section on self similar solution expanded, appendix removed, references added. To appear in Phys. Rev.D
dc.identifierhttps://arxiv.org/abs/0712.1413
dc.identifierhttp://arxiv.org/abs/0712.1413
dc.identifierPhys.Rev.D77:064012,2008
dc.identifierdoi:10.1103/PhysRevD.77.064012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199861
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleClassical and Quantum Gravitational Collapse in d-dim AdS Spacetime I. Classical Solutions
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