Geometric Horizons in the Kastor-Traschen Multi Black Hole Solutions
arXiv:1811.02931 · doi:10.1103/PhysRevD.98.064043
Abstract
We investigate the existence of invariantly defined quasi-local hypersurfaces in the Kastor-Traschen solution containing charge-equal-to-mass black holes. These hypersurfaces are characterized by the vanishing of particular curvature invariants, known as Cartan invariants, which are generated using the frame approach. The Cartan invariants of interest describe the expansion of the outgoing and ingoing null vectors belonging to the invariant null frame arising from the Cartan-Karlhede algorithm. We show that the evolution of the hypersurfaces surrounding the black holes depends on an upper-bound on the total mass for the case of two and three equal mass black holes. We discuss the results in the context of the geometric horizon conjectures.
arXiv comment24 pages, 17 figures
References in corpus (41)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Isolated and dynamical horizons and their applications
- General Laws of Black-Hole Dynamics
- Stationary Black Holes: Uniqueness and Beyond
- Dynamical Horizons and their Properties
- Dynamical Horizons: Energy, Angular Momentum, Fluxes and Balance Laws
- Mechanics of Rotating Isolated Horizons
- Black hole boundaries
- A 3+1 perspective on null hypersurfaces and isolated horizons
- Classification of the Weyl Tensor in Higher Dimensions
- Local existence of dynamical and trapping horizons
- Cosmological Multi-Black Hole Solutions
- Geometry of Generic Isolated Horizons
- Classification of the Weyl Tensor in Higher Dimensions and Applications
- Alignment and algebraically special tensors in Lorentzian geometry
- Spacetimes characterized by their scalar curvature invariants
- Isolated, slowly evolving, and dynamical trapping horizons: geometry and mechanics from surface deformations
- Testing Cosmic Censorship with Black Hole Collisions
- Global Structure of a Black-Hole Cosmos and its Extremes
- A Cosmological Constant Limits the Size of Black Holes
- Foliation dependence of black hole apparent horizons in spherical symmetry
- Trapped surfaces
- Dynamics of marginally trapped surfaces in a binary black hole merger: Growth and approach to equilibrium
- Invariant characterization of the Kerr spacetime: Locating the horizon and measuring the mass and spin of rotating black holes using curvature invariants
- Local Invariants Vanishing on Stationary Horizons: A Diagnostic for Locating Black Holes
- Curvature operators and scalar curvature invariants
- Geometric Horizons
- Identification of black hole horizons using scalar curvature invariants
- Scalar Polynomial Curvature Invariant Vanishing on the Event Horizon of Any Black Hole Metric Conformal to a Static Spherical Metric
- Exact Event Horizon of a Black Hole Merger
- Sources for the Majumdar-Papapetrou Space-Times
- Black hole fusion in the extreme mass ratio limit
- On marginally outer trapped surfaces in stationary and static spacetimes
- Spacetime invariants and their uses
- Algebraic classification of five-dimensional spacetimes using scalar invariants
- Curvature invariant characterization of event horizons of four-dimensional black holes conformal to stationary black holes
- Cartan Invariants and Event Horizon Detection, Extended Version
- Black hole formation from the gravitational collapse of a non-spherical network of structures
- Deformation of horizons during a merger
- A covariant Hamiltonian tetrad approach to numerical relativity
- Algebraic classification of spacetimes using discriminating scalar curvature invariants
Cited by in corpus (11)
- Charges and Fluxes on (Perturbed) Non-expanding Horizons
- Curvature Invariants and Lower Dimensional Black Hole Horizons
- Geometric surfaces: An invariant characterization of spherically symmetric black hole horizons and wormhole throats
- A Critical Assessment of Black Hole Solutions With a Linear Term in Their Redshift Function
- On the Curvature Invariants of the Massive Banados-Teitelboim-Zanelli Black Holes and Their Holographic Pictures
- Trapped region in Kerr-Vaidya space-time
- Geometric horizons in binary black hole mergers
- Persistence in black hole lattice cosmological models
- An invariant characterization of the quasi-spherical Szekeres dust models
- Geometric Horizons: A Frame Approach
- Alternative characterization of a black hole boundary