The study of gravitational collapse model in higher dimensional space-time

Abstract

We investigate the end state of the gravitational collapse of an inhomogeneous dust cloud in higher dimensional space-time. The naked singularities are shown to be developing as the final outcome of non-marginally bound collapse. The naked singularities are found to be gravitationally strong in the sense of Tipler .

6 Latex pages, No figure, Revtex style

Cited by in corpus (9)

• Final fate of spherically symmetric gravitational collapse of a dust cloud in Einstein-Gauss-Bonnet gravity
• Higher Dimensional Wormhole Geometries with Compact Dimensions
• Gravitational Collapse in Generalized Vaidya Space-Time for Lovelock Gravity Theory
• Thermodynamics of Lemaitre-Tolman-Bondi Model
• Emergent scenario and different anisotropic models
• Thermodynamics of the inhomogeneous perfect fluid LTB model: Modified Bekenstein-Hawking system
• Lemaitre-Tolman-Bondi model of the universe and Hawking radiation of a dynamical horizon
• The cosmic censorship conjecture in a higher dimensional spacetime with an interacting vacuum energy
• Brane Isotropisation in Extra-Dimensional Tolman-Bondi Universe