Novel Cauchy-horizon instability
arXiv:gr-qc/0501042 · doi:10.1103/PhysRevD.71.064015
Abstract
The evolution of weak discontinuity is investigated on horizons in the -dimensional static solutions in the Einstein-Maxwell-scalar- system, including the Reissner-Nordström-(anti) de Sitter black hole. The analysis is essentially local and nonlinear. We find that the Cauchy horizon is unstable, whereas both the black-hole event horizon and the cosmological event horizon are stable. This new instability, the so-called kink instability, of the Cauchy horizon is completely different from the well-known ``infinite-blueshift'' instability. The kink instability makes the analytic continuation beyond the Cauchy horizon unstable.
6 pages, 1 figure, final version to appear in Physical Review D
References in corpus (2)
Cited by in corpus (21)
- Spacetime structure of static solutions in Gauss-Bonnet gravity: neutral case
- Bulk and Brane Decay of a (4+n)-Dimensional Schwarzschild-De-Sitter Black Hole: Scalar Radiation
- Spacetime structure of static solutions in Gauss-Bonnet gravity: charged case
- Towards a Non-singular Paradigm of Black Hole Physics
- Non-polynomial Lagrangian approach to Regular Black Holes
- A special class of solutions in -gravity
- Observational Constraints in Metric-Affine Gravity
- AdS-Taub-NUT spacetimes and exact black bounces with scalar hair
- Semiclassical instability of inner-extremal regular black holes
- Distorted Five-dimensional Electrically Charged Black Holes
- Plebański-Demiański solutions with dynamical torsion and nonmetricity fields
- Topological regular black holes without Cauchy horizon
- Mass inflation inside black holes revisited
- Black hole nonmodal linear stability: odd perturbations of Reissner-Nordström
- Nonsingular Black Holes From Charged Dust Collapse: A Concrete Mechanism to Evade Interior Singularities in General Relativity
- Black hole nonmodal linear stability: even perturbations in the Reissner-Nordström case
- Charged Black Holes from Interacting Vacuum
- Perturbation theory of spherically symmetric self-similar black holes
- Distinguish Bardeen-like black holes by Gravitational lensing
- On the Stability of a Wormhole in the Maximally-Extended Reissner-Nordström Solution
- A no-go theorem for regular black holes