Singularity in Gravitational Collapse of Plane Symmetric Charged Vaidya Spacetime
arXiv:1006.3595 · doi:10.1142/S0217732310033864
Abstract
We study the final outcome of gravitational collapse resulting from the plane symmetric charged Vaidya spacetime. Using the field equations, we show that the weak energy condition is always satisfied by collapsing fluid. It is found that the singularity formed is naked. The strength of singularity is also investigated by using Nolan's method. This turns out to be a strong curvature singularity in Tipler's sense and hence provides a counter example to the cosmic censorship hypothesis.
arXiv comment8 pages, accepted for publication in Mod. Phys. Lett A
References in corpus (16)
- Schwarzschild black hole lensing
- The geometry of photon surfaces
- Relativistic images of Schwarzschild black hole lensing
- Time delay and magnification centroid due to gravitational lensing by black holes and naked singularities
- Naked singularities and Seifert's conjecture
- Why do naked singularities form in gravitational collapse?
- Role of the scalar field in gravitational lensing
- Spherical gravitational collapse in N-dimensions
- Collapsing strange quark matter in Vaidya geometry
- Collapsing shells of radiation in anti-de Sitter spacetimes and the hoop and cosmic censorship conjectures
- Gravitational Perfect Fluid Collapse With Cosmological Constant
- Effects of Electromagnetic Field on Gravitational Collapse
- Effects of the Electromagnetic Field on Five-dimensional Gravitational Collapse
- High-Speed Cylindrical Collapse of Two Perfect Fluids
- Gravitational Charged Perfect Fluid Collapse in Friedmann Universe Models
- Charged null fluid collapse in anti-de Sitter spacetimes and naked singularities