The role of the equation of state and the space-time dimension in spherical collapse
arXiv:gr-qc/0305088 · doi:10.1142/S0217751X05021038
Abstract
We study the spherically symmetric collapse of a fluid with non-vanishing radial pressure in higher dimensional space-time. We obtain the general exact solution in the closed form for the equation of state () which leads to the explicit construction of the root equation governing the nature (black hole versus naked singularity) of the central singularity. A remarkable feature of the root equation is its invariance for the three cases: (), () and () where is the dimension of space-time. That is, for the ultimate end result of the collapse, -dimensional dust, - AdS (anti de Sitter)-like and - dS-like are absolutely equivalent.
arXiv comment4 Pages, RevTeX, no figures, minor changes, new references added, Detailed version to follow
References in corpus (13)
- A Large Mass Hierarchy from a Small Extra Dimension
- Naked Singularities in Spherically Symmetric Inhomogeneous Tolman-Bondi Dust Cloud Collapse
- On the Role of Initial Data in the Gravitational Collapse of Inhomogeneous Dust
- Final fate of the spherically symmetric collapse of a perfect fluid
- On naked singularities in higher dimensional Vaidya space-times
- Naked singularity formation in the collapse of a spherical cloud of counterrotating particles
- Higher dimensional inhomogeneous dust collapse and cosmic censorship
- Negative Pressure and Naked Singularities in Spherical Gravitational Collapse
- Black holes vs. naked singularities formation in collapsing Einstein's clusters
- Gravitational collapse of Type II fluid in higher dimensional space-times
- Gravitational Collapse of Perfect Fluid
- Singularities in gravitational collapse with radial pressure
- Gravitational Collapse of Perfect Fluid in N-Dimensional Spherically Symmetric Spacetimes
Cited by in corpus (6)
- Final fate of spherically symmetric gravitational collapse of a dust cloud in Einstein-Gauss-Bonnet gravity
- Bardeen-like regular black holes in Einstein-Gauss-Bonnet gravity
- Is cosmic censorship restored in higher dimensions?
- Charged compact star model in Einstein-Maxwell-Gauss-Bonnet gravity
- Spherically symmetric solutions and gravitational collapse in brane-worlds
- The effect of loop quantum gravitational rainbow functions on the formation of naked singularities