Tolman-Bondi Space-Time in Brane World Scenario

dc.creatorChakraborty, Subenoy
dc.creatorBanerjee, Asit
dc.creatorDebnath, Ujjal
dc.date2006-02-17
dc.date.accessioned2026-07-07T07:02:37Z
dc.date.available2026-07-07T07:02:37Z
dc.descriptionIn the present work, inhomogeneous Tolman-Bondi type dust space-time is studied on the brane. There are two sets of solutions of the above model. The first solution represents either a collapsing model starting from an infinite volume at infinite past to the singularity or a model starting from a singularity and expanding for ever having a transition from decelerating phase to accelerating phase. The first solution shows that the end state of collapse may be black hole or a naked singularity depending signs of various parameters involved. The second solution represents a bouncing model where the bounce occurs at different comoving radii at different epochs.
dc.description6 Latex pages, RevTeX style, 3 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0602068
dc.identifierhttp://arxiv.org/abs/gr-qc/0602068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108670
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTolman-Bondi Space-Time in Brane World Scenario
dc.typetext

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