Gravitational Collapse in Higher Dimension

Abstract

Spherically symmetric inhomogeneous dust collapse has been studied in higher dimensional space-time and appearance of naked singularity has been analyzed both for non-marginal and marginally bound cases. It has been shown that naked singularity is possible for any arbitrary dimension in non-marginally bound case. For marginally bound case we have examined the radial null geodesics from the singularity and found that naked singularity is possible upto five dimension.

8 Latex pages, No figure, Revtex style

References in corpus (6)

• Why do naked singularities form in gravitational collapse?
• Physical Processes in Naked Singularity Formation
• On naked singularities in higher dimensional Vaidya space-times
• Naked Singularities in Higher Dimensional Gravitational Collapse
• Higher dimensional inhomogeneous dust collapse and cosmic censorship
• Non-marginally bound inhomogeneous dust collapse in higher dimensional space-time

Cited by in corpus (13)

• Final fate of spherically symmetric gravitational collapse of a dust cloud in Einstein-Gauss-Bonnet gravity
• Gravitational Collapse in Generalized Vaidya Space-Time for Lovelock Gravity Theory
• Thermodynamics of Lemaitre-Tolman-Bondi Model
• Trapped surfaces and nature of singularities in Lyra's geometry
• Emergent scenario and different anisotropic models
• Naked Singularities in Higher Dimensional Szekeres Space-time
• Gravitational Collapse With Dark Energy And Dark Matter In Hořava-Lifshitz Gravity
• Fluid pulsation modes from strange stars in a higher-dimensional space-time
• The effect of Pressure in Higher Dimensional Quasi-Spherical Gravitational Collapse
• Dimensional dependence of naked singularity formation in spherical gravitational collapse
• 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
• Brane Isotropisation in Extra-Dimensional Tolman-Bondi Universe