Strong curvature naked singularities in spherically symmetric perfect fluid collapse
arXiv:2001.04367 · doi:10.1103/PhysRevD.101.044052
Abstract
We investigate here the locally naked singularity formed due to a spherically symmetric inhomogeneous collapsing cloud having non-zero isotropic pressure, in terms of its strength. Sufficient condition provided by Clarke and Krolak for it to be Tipler strong has been used to restrict the parameters that represent the non-linear relation between the physical radius and the radial coordinate of the outgoing radial null geodesic at the singular center. Studying end state of a collapsing cloud requires information about the dynamics of collapse, which is unknown in a general scenario. Hence we study small perturbations to the mass profile for inhomogeneous dust, which is possible using the formalism developed here. This perturbed mass profile, in turn, gives rise to non-zero pressure. We show the existence of a non-zero measure set of initial data giving rise to such strong curvature naked singularity.
arXiv comment8 pages
References in corpus (14)
- Naked Singularities in Spherically Symmetric Inhomogeneous Tolman-Bondi Dust Cloud Collapse
- Recent developments in gravitational collapse and spacetime singularities
- The Final Fate of Spherical Inhomogeneous Dust Collapse
- The state space and physical interpretation of self-similar spherically symmetric perfect-fluid models
- Spherical gravitational collapse in N-dimensions
- Gravitational collapse with non-vanishing tangential stresses II: a laboratory for cosmic censorship experiments
- New solutions of Einstein equations in spherical symmetry: the Cosmic Censor to the court
- Gravitational collapse of an isentropic perfect fluid with a linear equation of state
- Nakedness and curvature strength of shell-focusing singularity in the spherically symmetric space-time with vanishing radial pressure
- Gravitational collapse of barotropic spherical fluids
- Genericity aspects in gravitational collapse to black holes and naked singularities
- The Central Singularity in Spherical Collapse
- Strong curvature singularities in quasispherical asymptotically de Sitter dust collapse
- Instability of black hole formation under small pressure perturbations
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