Symmetric non-expanding horizons
arXiv:gr-qc/0605026 · doi:10.1088/0264-9381/23/20/022
Abstract
Symmetric non-expanding horizons are studied in arbitrary dimension. The global properties -as the zeros of infinitesimal symmetries- are analyzed particularly carefully. For the class of NEH geometries admitting helical symmetry a quasi-local analog of Hawking's rigidity theorem is formulated and proved: the presence of helical symmetry implies the presence of two symmetries: null, and cyclic. The results valid for arbitrary-dimensional horizons are next applied in a complete classification of symmetric NEHs in 4-dimensional space-times (the existence of a 2-sphere crossection is assumed). That classification divides possible NEH geometries into classes labeled by two numbers - the dimensions of, respectively, the group of isometries induced in the horizon base space and the group of null symmetries of the horizon.
Revtex4, 36 pages
References in corpus (37)
- A rotating black ring in five dimensions
- Isolated and dynamical horizons and their applications
- General Laws of Black-Hole Dynamics
- Unified first law of black-hole dynamics and relativistic thermodynamics
- Dynamical Horizons and their Properties
- Dynamical Horizons: Energy, Angular Momentum, Fluxes and Balance Laws
- Generic Isolated Horizons and their Applications
- Mechanics of Rotating Isolated Horizons
- Black hole boundaries
- Dynamic black-hole entropy
- Geometry of Generic Isolated Horizons
- Mechanics of Isolated Horizons
- Isolated Horizons: A Generalization of Black Hole Mechanics
- The first law for slowly evolving horizons
- Energy and entropy conservation for dynamical black holes
- Gravitational waves in general relativity: XIV. Bondi expansions and the ``polyhomogeneity'' of \Scri
- A boundary value problem for the five-dimensional stationary rotating black holes
- On non-existence of static vacuum black holes with degenerate components of the event horizon
- Extremal Isolated Horizons: A Local Uniqueness Theorem
- Energy conservation for dynamical black holes
- Space-Times Admitting Isolated Horizons
- Spin-Coefficient Form of the New Laws of Black-Hole Dynamics
- Quasi-local rotating black holes in higher dimension: geometry
- Quasi-local first law of black-hole dynamics
- Mechanics of multidimensional isolated horizons
- Horizon energy and angular momentum from a Hamiltonian perspective
- Metric-based Hamiltonians, null boundaries, and isolated horizons
- Spacetimes foliated by Killing horizons
- Geometric Characterizations of the Kerr Isolated Horizon
- Uniqueness theorem for stationary black hole solutions of σ-models in five dimensions
- Dynamics of a self gravitating light-like matter shell: a gauge-invariant Lagrangian and Hamiltonian description
- Boundary Terms and Noether Current of Sphereical Black Holes
- Gravitational radiation from dynamical black holes
- Dynamics of gravitational field within a wave front and thermodynamics of black holes
- Intrinsic Geometry of a Null Hypersurface
- Geometry of null hypersurfaces
- Local approach to thermodynamics of black holes
Cited by in corpus (20)
- Isolated, slowly evolving, and dynamical trapping horizons: geometry and mechanics from surface deformations
- Black holes and black hole thermodynamics without event horizons
- Charges and Fluxes on (Perturbed) Non-expanding Horizons
- The spacetime in the neighborhood of a general isolated black hole
- Non-Expanding horizons: Multipoles and the Symmetry Group
- Asymptotics with a positive cosmological constant: IV. The `no-incoming radiation' condition
- Quasi--local angular momentum of non--symmetric isolated and dynamical horizons from the conformal decomposition of the metric
- Local version of the no-hair theorem
- Multiple Killing Horizons
- The Petrov type D isolated null surfaces
- Neighbourhoods of Isolated Horizons and their stationarity
- Some spacetimes containing non-rotating extremal isolated horizons
- Vacuum non-expanding horizons and shear-free null geodesic congruences
- Projectively non-singular horizons in Kerr-NUT-de Sitter spacetimes
- Non-singular Kerr-NUT-de Sitter spacetimes
- Kerr Isolated Horizons in Ashtekar and Ashtekar-Barbero Connection Variables
- Petrov type D equation on horizons of nontrivial bundle topology
- Initial data for a deformed isolated horizon
- On Super-Translation transition between Quasi-local Black holes
- Vacuum Petrov type D horizons of non-trivial bundle structure over Riemann surfaces with genus