What Happens to Apparent Horizons in a Binary Black Hole Merger?
arXiv:2104.10265 · doi:10.1103/PhysRevLett.127.181101
Abstract
We resolve the fate of the two original apparent horizons during the head-on merger of two non-spinning black holes. We show that following the appearance of the outer common horizon and subsequent inter-penetration of the original horizons, they continue to exist for a finite period of time before they are individually annihilated by unstable MOTSs. The inner common horizon vanishes in a similar, though independent, way. This completes the understanding of the analogue of the event horizon's "pair of pants" diagram for the apparent horizon. Our result is facilitated by a new method for locating marginally outer trapped surfaces (MOTSs) based on a generalized shooting method. We also discuss the role played by the MOTS stability operator in discerning which among a multitude of MOTSs should be considered as black hole boundaries.
6 pages, 5 figures, V2: final version with several changes (including changed title)
References in corpus (5)
- Understanding the "anti-kick" in the merger of binary black holes
- The time evolution of marginally trapped surfaces
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Cited by in corpus (15)
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- Tidal deformation of dynamical horizons in binary black hole mergers
- Quasi-Local Black Hole Horizons: Recent Advances
- Symmetry and instability of marginally outer trapped surfaces
- Extreme Gravitational Interactions in the Problem of Three Black Holes in General Relativity
- Exotic marginally outer trapped surfaces in rotating spacetimes of any dimension
- Properties of Quasi-local mass in binary black hole mergers
- Marginally Outer Trapped Tori in Black Hole Spacetimes
- On the existence of conformal Killing horizons in LRS spacetimes
- Ultimate fate of apparent horizons during a binary black hole merger I: Locating and understanding axisymmetric marginally outer trapped surfaces
- Dynamical Horizon Segments and Spacetime Isometries
- Revisiting the apparent horizon finding problem with multigrid methods
- Entangled universes
- The Interior MOTSs of Spherically Symmetric Black Holes
- Black holes and their horizons in semiclassical and modified theories of gravity