Radiation collapse and gravitational waves in three dimensions
arXiv:gr-qc/9404047 · doi:10.1103/PhysRevD.50.R2361
Abstract
Two non-static solutions for three dimensional gravity coupled to matter fields are given. One describes the collapse of radiation that results in a black hole. This is the three dimensional analog of the Vaidya metric, and is used to construct a model for mass inflation. The other describes plane gravitational waves for coupling to a massless scalar field.
9 pages (RevTeX) 1 figure upon request, Alberta-Thy-12-94
Cited by in corpus (31)
- Scalar Wave Falloff in Asymptotically Anti-de Sitter Backgrounds
- Conformally dressed black hole in 2+1 dimensions
- Gravitational collapse in 2+1 dimensional AdS spacetime
- Scalar field collapse in three-dimensional AdS spacetime
- On the fate of quantum black holes
- Energy and Momentum Distributions of a (2+1)-dimensional black hole background
- Beyond the veil: Inner horizon instability and holography
- Collapse of a Scalar Field in 2+1 Gravity
- Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities
- Interior Structure of a Charged Spinning Black Hole in -Dimensions
- Quantum-corrected black holes and naked singularities in (2+1)-dimensions
- All solutions of Einstein's equations in 2+1 dimensions: -vacuum, pure radiation, or gyratons
- Black hole solutions in 2+1 dimensions
- Mass inflation in (1+1)-dimensional Dilaton Gravity
- Holographic description of asymptotically AdS_2 collapse geometries
- Extracting information behind the veil of horizon
- Mass inflation and strong cosmic censorship in a non-extreme BTZ black hole
- Blushift of a tachyon in the charged 2D black hole
- Charged Rotating Black Hole Formation from Thin Shell Collapse in Three Dimensions
- Domain Wall Spacetimes: Instability of Cosmological Event and Cauchy Horizons
- Inside a Spinning Black String
- Is BTZ a separate superselection sector of CTMG?
- Exact black-hole formation with a conformally coupled scalar field in three dimensions
- A Toy Penrose Inequality and its Proof
- Moving mirrors and event horizons in non-flat background geometry
- Gravitational collapse of a circularly symmetric star
- Gravitational Collapse of Massless Scalar Field with Negative Cosmological Constant in (2+1) Dimensions
- Investigations of strong cosmic censorship in 3-dimensional black strings
- Linearized 3D gravity with dust
- Thermodynamical and dynamical stability of Einstein-Maxwell and extremal Einstein-Born-Infeld thin shells in dimensions
- Ultra-massive spacetimes in 2+1 dimensions with positive Λ