Approximate Killing Vectors on S^2
arXiv:0706.0199 · doi:10.1103/PhysRevD.76.041501
Abstract
We present a new method for computing the best approximation to a Killing vector on closed 2-surfaces that are topologically S^2. When solutions of Killing's equation do not exist, this method is shown to yield results superior to those produced by existing methods. In addition, this method appears to provide a new tool for studying the horizon geometry of distorted black holes.
4 pages, 3 figures, submitted to Physical Review D, revtex4
References in corpus (7)
- Quasilocal Energy and Conserved Charges Derived from the Gravitational Action
- Isolated and dynamical horizons and their applications
- Introduction to Isolated Horizons in Numerical Relativity
- Spin Flips and Precession in Black-Hole-Binary Mergers
- Circular orbits and spin in black-hole initial data
- Introduction to dynamical horizons in numerical relativity
- Angular momentum conservation for dynamical black holes
Cited by in corpus (60)
- The SXS Collaboration catalog of binary black hole simulations
- High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions
- High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
- Binary-black-hole initial data with nearly-extremal spins
- Gravitational waves from spinning black hole-neutron star binaries: dependence on black hole spins and on neutron star equations of state
- Simulations of non-equal mass black hole binaries with spectral methods
- Improved methods for simulating nearly extremal binary black holes
- Angular velocity of gravitational radiation from precessing binaries and the corotating frame
- Simulating merging binary black holes with nearly extremal spins
- Foundations of multiple black hole evolutions
- Initial data for black hole-neutron star binaries: a flexible, high-accuracy spectral method
- Modeling the source of GW150914 with targeted numerical-relativity simulations
- High accuracy simulations of black hole binaries:spins anti-aligned with the orbital angular momentum
- Extremality conditions for isolated and dynamical horizons
- Coalescence of black hole--neutron star binaries
- Intermediate mass-ratio black hole binaries: Applicability of small mass-ratio perturbation theory
- The spin expansion for binary black hole merger: new predictions and future directions
- Relativistic black hole-neutron star binaries in quasiequilibrium: effects of the black hole excision boundary condition
- Binary Neutron Stars with Arbitrary Spins in Numerical Relativity
- Mass and Angular Momentum in General Relativity
- Reducing spurious gravitational radiation in binary-black-hole simulations by using conformally curved initial data
- Dynamics of marginally trapped surfaces in a binary black hole merger: Growth and approach to equilibrium
- From Geometry to Numerics: interdisciplinary aspects in mathematical and numerical relativity
- Comparing Post-Newtonian and Numerical-Relativity Precession Dynamics
- Nearly extremal apparent horizons in simulations of merging black holes
- Motion in classical field theories and the foundations of the self-force problem
- Approximate spacetime symmetries and conservation laws
- Quasi-Local Linear Momentum in Black-Hole Binaries
- The Final Remnant of Binary Black Hole Mergers: Multipolar Analysis
- Visualizing Spacetime Curvature via Frame-Drag Vortexes and Tidal Tendexes II. Stationary Black Holes
- Quasiequilibrium states of black hole-neutron star binaries in the moving-puncture framework
- Redshift factor and the first law of binary black hole mechanics in numerical simulations
- The spacetime in the neighborhood of a general isolated black hole
- An introduction to local Black Hole horizons in the 3+1 approach to General Relativity
- Dynamical Black Holes: Approach to the Final State
- Comparing Remnant Properties from Horizon Data and Asymptotic Data in Numerical Relativity
- Targeted numerical simulations of binary black holes for GW170104
- Horizon dynamics of distorted rotating black holes
- Fundamental properties and applications of quasi-local black hole horizons
- Horizon Surface Gravity in Corotating Black Hole Binaries
- A Proposal for Determining the Energy Content of Gravitational Waves by Using Approximate Symmetries of Differential Equations
- A new method to compute quasi-local spin and other invariants on marginally trapped surfaces
- Quasi--local angular momentum of non--symmetric isolated and dynamical horizons from the conformal decomposition of the metric
- Initial data for black hole-neutron star binaries, with rotating stars
- Perturbative stability of the approximate Killing field eigenvalue problem
- Seeking for toroidal event horizons from initially stationary BH configurations
- Black Hole Spin Axis in Numerical Relativity
- Total angular momentum from Dirac eigenspinors
- Approximate Killing Fields as an Eigenvalue Problem
- Definitions of (super) angular momentum in asymptotically flat spacetimes: Properties and applications to compact-binary mergers
- Phenomenological gravitational waveform model of binary black holes incorporating horizon fluxes
- Tidal deformations of spinning black holes in Bowen-York initial data
- Horizons as boundary conditions in spherical symmetry
- Approximate Killing symmetries in non-perturbative quantum gravity
- Hidden Killing Fields, Geometric Symmetries and Black Hole Mergers
- Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework
- Isometric embeddings of 2-spheres by embedding flow for applications in numerical relativity
- Quasi-local spin-angular momentum and the construction of axial vector fields
- Decline of the current quadrupole moment during the merger phase of binary black hole coalescence
- Redshift factor and the small mass-ratio limit in binary black hole simulations