Ultra-massive spacetimes in 2+1 dimensions with positive Λ
arXiv:2503.19187 · doi:10.1088/1361-6382/addc2e
Abstract
We show that ultra-massive spacetimes exist also in 2 + 1 dimensions with a positive cosmological constant Λ > 0. They can be created through the collapse of a spherical null dust shell. The exterior of the shell is then a Mess spacetime, that is to say a locally de Sitter spacetime that cannot be obtained as a quotient of de Sitter space.
arXiv comment16 pages, 5 figures. Minor corrections and improved discussion. Matches published version
References in corpus (18)
- The Black Hole in Three Dimensional Space Time
- The (2+1)-Dimensional Black Hole
- Singularity Theorems and Their Consequences
- Black hole boundaries
- Local existence of dynamical and trapping horizons
- No Black Hole Theorem in Three-Dimensional Gravity
- Axial symmetry and conformal Killing vectors
- The region with trapped surfaces in spherical symmetry, its core, and their boundaries
- Trapped surfaces and symmetries
- A Cosmological Constant Limits the Size of Black Holes
- Trapped surfaces
- Singularity theorems based on trapped submanifolds of arbitrary co-dimension
- Radiation collapse and gravitational waves in three dimensions
- Bounded Area Theorems for Higher Genus Black Holes
- Bounds on area and charge for marginally trapped surfaces with cosmological constant
- Black hole solutions in 2+1 dimensions
- De Sitter Space and Spatial Topology
- Nonexistence of marginally trapped surfaces and geons in 2+1 gravity