Black hole singularities: a new critical phenomenon
arXiv:gr-qc/0209084 · doi:10.1103/PhysRevLett.90.121101
Abstract
The singularitiy inside a spherical charged black hole, coupled to a spherical, massless scalar field is studied numerically. The profile of the characteristic scalar field was taken to be a power of advanced time with an exponent . A critical exponent exists. For exponents below the critical one () the singularity is a union of spacelike and null sectors, as is also the case for data with compact support. For exponents greater than the critical one () an all-encompassing, spacelike singularity evolves, which completely blocks the ``tunnel'' inside the black hole, preventing the use of the black hole as a portal for hyperspace travel.
4 pages, 5 eps figures; An Erratum is added. The main conclusions of the original Letter are unchanged
References in corpus (2)
Cited by in corpus (27)
- Critical phenomena in gravitational collapse
- Classes of Exact Solutions to the Teukolsky Master Equation
- Exploring New Physics Frontiers Through Numerical Relativity
- The physics of the relativistic counter-streaming instability that drives mass inflation inside black holes
- Passage of radiation through wormholes
- Outgoing gravitational shock-wave at the inner horizon: The late-time limit of black hole interiors
- Late-time evolution of charged massive Dirac fields in the Reissner-Nordström black-hole background
- Physics of the interior of a spherical, charged black hole with a scalar field
- Novel Cauchy-horizon instability
- Interior of a Charged Distorted Black Hole
- Mass Inflation in Brans-Dicke gravity
- Accretion with back reaction
- Hawking radiation inside a charged black hole
- Physics of the interior of a black hole with an exotic scalar matter
- The interior structure of rotating black holes 2. Uncharged black holes
- Inside charged black holes II. Baryons plus dark matter
- Is it possible to see the infinite future of the Universe when falling into a black hole?
- Geometry near the inner horizon of a rotating, accreting black hole
- Distorted stationary rotating black holes
- Mass inflation in a D dimensional Reissner-Nordstrom black hole: a hierarchy of particle accelerators ?
- Inside charged black holes I. Baryons
- Renormalization of at the inner horizon of rotating, accreting black holes
- Black hole nonmodal linear stability: odd perturbations of Reissner-Nordström
- Gravitational shock wave inside a steadily-accreting spherical charged black hole
- Charged Black Holes from Interacting Vacuum
- Perturbation theory of spherically symmetric self-similar black holes
- Revisiting Schwarzschild black hole singularity through string theory