Do Naked Singularities Form?
arXiv:gr-qc/9511018 · doi:10.1088/0264-9381/13/5/004
Abstract
A naked singularity is formed by the collapse of a Sine-Gordon soliton in 1+1 dimensional dilaton gravity with a negative cosmological constant. We examine the quantum stress tensor resulting from the formation of the singularity. Consistent boundary conditions require that the incoming soliton is accompanied by a flux of incoming radiation across past null infinity, but neglecting the back reaction of the spacetime leads to the absurd conclusion that the total energy entering the system by the time the observer is able to receive information from the singularity is infinite. We conclude that the back reaction must prevent the formation of the naked singularity.
7 pages (21 Kb), PHYZZX. Revised version to appear in Class. & Quant. Grav. Letts. A discussion of the consistency of the Sine-Gordon model is included
References in corpus (4)
Cited by in corpus (13)
- Initial data and the end state of spherically symmetric gravitational collapse
- Particle Creation in the Marginally Bound, Self Similar Collapse of Inhomogeneous Dust
- The Quantum Stress-Tensor in Self-Similar Spherical Dust Collapse
- K-field kinks in two-dimensional dilaton gravity
- Quantum Naked Singularities in 2d Dilaton Gravity
- Runaway Collapse of Witten Vortex Loops
- Revisit on two-dimensional self-gravitating kinks: superpotential formalism and linear stability
- Normal modes for two-dimensional gravitating kinks
- Gravitational Collapse of Baryonic and Dark matter
- Kink solutions in generalized 2D dilaton gravity
- Differential configurational entropy for multi-field of the theory
- Unveiling horizons in quantum critical collapse
- Energy emission from high curvature region and its backreation