Notes on Cosmic Censorship Conjecture revisited: Covariantly
arXiv:1604.01157
Abstract
In this paper we study the dynamics of the trapped region using a frame independent semi-tetrad covariant formalism for general Locally Rotationally Symmetric (LRS) class II spacetimes. We covariantly prove some important geometrical results for the apparent horizon, and state the necessary and sufficient conditions for a singularity to be locally naked. These conditions bring out, for the first time in a quantitative and transparent manner, the importance of the Weyl curvature in deforming and delaying the trapped region during continual gravitational collapse, making the central singularity locally visible.
arXiv comment6 pages, Conference proceeding for MG14, submitted to MG14 2015, based on arXiv:1402.4355
References in corpus (9)
- Why do naked singularities form in gravitational collapse?
- A covariant approach for perturbations of rotationally symmetric spacetimes
- Covariant Perturbations of Schwarzschild Black Holes
- Scalar Perturbations on Lemaitre-Tolman-Bondi Spacetimes
- Spherical gravitational collapse in N-dimensions
- A Geometrical Approach to Strong Gravitational Lensing in f(R) Gravity
- Spherical Dust Collapse in Higher Dimensions
- Cosmic Censorship in Higher dimension II
- Gravitational Lensing in Spherically Symmetric Spacetimes