A geometrically motivated coordinate system for exploring spacetime dynamics in numerical-relativity simulations using a quasi-Kinnersley tetrad
arXiv:1208.0630 · doi:10.1103/PhysRevD.86.084020
Abstract
We investigate the suitability and properties of a quasi-Kinnersley tetrad and a geometrically motivated coordinate system as tools for quantifying both strong-field and wave-zone effects in numerical relativity (NR) simulations. We fix the radial and latitudinal coordinate degrees of freedom of the metric, using the Coulomb potential associated with the quasi-Kinnersley transverse frame. These coordinates are invariants of the spacetime and can be used to unambiguously fix the outstanding spin-boost freedom associated with the quasi-Kinnersley frame (resulting in a preferred quasi-Kinnersley tetrad (QKT)). In the limit of small perturbations about a Kerr spacetime, these coordinates and QKT reduce to Boyer-Lindquist coordinates and the Kinnersley tetrad, irrespective of the simulation gauge choice. We explore the properties of this construction both analytically and numerically, and we gain insights regarding the propagation of radiation described by a super-Poynting vector. We also quantify in detail the peeling properties of the chosen tetrad and gauge. We argue that these choices are particularly well suited for a rapidly converging wave-extraction algorithm as the extraction location approaches infinity, and we explore numerically the extent to which this property remains applicable on the interior of a computational domain. Using a number of additional tests, we verify that the prescription behaves as required in the appropriate limits regardless of simulation gauge. We explore the behavior of the geometrically motivated coordinate system in dynamical binary-black-hole NR mergers, and find them useful for visualizing features in NR simulations such as the spurious "junk" radiation. Finally, we carefully scrutinize the head-on collision of two black holes and, for example, the way in which the extracted waveform changes as it moves through the computational domain.
30 pages, 17 figures, 2 tables
References in corpus (35)
- Evolution of Binary Black Hole Spacetimes
- High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
- Gravito-electromagnetism
- Black-hole binaries, gravitational waves, and numerical relativity
- Simulation of Binary Black Hole Spacetimes with a Harmonic Evolution Scheme
- Tracking the precession of compact binaries from their gravitational-wave signal
- Modeling gravitational radiation from coalescing binary black holes
- High-powered Gravitational News
- A geometric approach to the precession of compact binaries
- Gauge invariant perturbations of Schwarzschild black holes in horizon-penetrating coordinates
- The Head-On Collision of Two Equal Mass Black Holes Peter Anninos
- Characteristic extraction in numerical relativity: binary black hole merger waveforms at null infinity
- Efficient asymptotic frame selection for binary black hole spacetimes using asymptotic radiation
- Frame-Dragging Vortexes and Tidal Tendexes Attached to Colliding Black Holes: Visualizing the Curvature of Spacetime
- Visualizing Spacetime Curvature via Frame-Drag Vortexes and Tidal Tendexes I. General Theory and Weak-Gravity Applications
- An Improved Gauge Driver for the Generalized Harmonic Einstein System
- A Characteristic Extraction Tool for Gravitational Waveforms
- Gravitational waves from black hole collisions via an eclectic approach
- The Lazarus Project. II. Spacelike extraction with the quasi-Kinnersley tetrad
- Characteristic Evolution and Matching
- Black hole head-on collisions and gravitational waves with fixed mesh-refinement and dynamic singularity excision
- Making use of geometrical invariants in black hole collisions
- Wave zone extraction of gravitational radiation in three-dimensional numerical relativity
- Towards wave extraction in numerical relativity: the quasi-Kinnersley frame
- Towards a novel wave-extraction method for numerical relativity. I. Foundations and initial-value formulation
- Algebraic Classification of Numerical Spacetimes and Black-Hole-Binary Remnants
- Mach's principle: Exact frame-dragging via gravitomagnetism in perturbed Friedmann-Robertson-Walker universes with
- The Status of Black-Hole Binary Merger Simulations with Numerical Relativity
- Gauge Drivers for the Generalized Harmonic Einstein Equations
- Towards a wave-extraction method for numerical relativity: IV. Testing the quasi-Kinnersley method in the Bondi-Sachs framework
- Spectral methods for the wave equation in second-order form
- Towards a wave--extraction method for numerical relativity: III. Analytical examples for the Beetle--Burko radiation scalar
- Classifying the Isolated Zeros of Asymptotic Gravitational Radiation by Tendex and Vortex Lines
- Degeneracy measures for the algebraic classification of numerical spacetimes
- Towards a wave-extraction method for numerical relativity. V. Extracting the Weyl scalars in the quasi-Kinnersley tetrad from spatial data
Cited by in corpus (14)
- Exploring New Physics Frontiers Through Numerical Relativity
- Numerical Relativity of Compact Binaries in the 21st Century
- The numerical relativity breakthrough for binary black holes
- Challenges in Quasinormal Mode Extraction: Perspectives from Numerical solutions to the Teukolsky Equation
- Extending Gravitational Wave Extraction Using Weyl Characteristic Fields
- Spectral Cauchy-characteristic extraction of the gravitational wave news function
- Stability of exact force-free electrodynamic solutions and scattering from spacetime curvature
- A joint approach for reducing eccentricity and spurious gravitational radiation in binary black hole initial data construction
- Black Hole Spin Axis in Numerical Relativity
- Gravitational wave extraction in higher dimensional numerical relativity using the Weyl tensor
- Spin coefficients and gauge fixing in the Newman-Penrose formalism
- Quasilocal energy exchange and the null cone
- Decline of the current quadrupole moment during the merger phase of binary black hole coalescence
- Local and Approximate classification of spacetimes in the transverse frames