The effect of Pressure in Higher Dimensional Quasi-Spherical Gravitational Collapse
arXiv:gr-qc/0604090 · doi:10.1142/S0218271807010432
Abstract
We study gravitational collapse in higher dimensional quasi-spherical Szekeres space-time for matter with anisotropic pressure. Both local and global visibility of central curvature singularity has been studied and it is found that with proper choice of initial data it is possible to show the validity of CCC for six and higher dimensions. Also the role of pressure in the collapsing process has been discussed.
arXiv comment11 pages, 6 figures, RevTeX style
References in corpus (11)
- Initial data and the end state of spherically symmetric gravitational collapse
- On the Occurrence of Naked Singularity in Spherically Symmetric Gravitational Collapse
- Final fate of the spherically symmetric collapse of a perfect fluid
- Naked Singularities in Higher Dimensional Gravitational Collapse
- What role pressures play to determine the final end-state of gravitational collapse?
- Gravitational collapse of an isentropic perfect fluid with a linear equation of state
- Quasi-Spherical Gravitational Collapse in Any Dimension
- Non-adiabatic collapse of a quasi-spherical radiating star
- Gravitational Collapse in Higher Dimension
- Spherical Universes with Anisotropic Pressure
- A study of higher dimensional inhomogeneous cosmological model