A new method to compute quasi-local spin and other invariants on marginally trapped surfaces
arXiv:0906.1228 · doi:10.1088/0264-9381/26/24/245008
Abstract
We accurately compute the scalar 2-curvature, the Weyl scalars, associated quasi-local spin, mass and higher multipole moments on marginally trapped surfaces in numerical 3+1 simulations. To determine the quasi-local quantities we introduce a new method which requires a set of invariant surface integrals, allowing for surface grids of a few hundred points only. The new technique circumvents solving the Killing equation and is also an alternative to approximate Killing vector fields. We apply the method to a perturbed non-axisymmetric black hole ringing down to Kerr and compare the quasi-local spin with other methods that use Killing vector fields, coordinate vector fields, quasinormal ringing and properties of the Kerr metric on the surface. Interesting is the agreement with the spin of approximate Killing vector fields during the phase of perturbed axisymmetry. Additionally, we introduce a new coordinate transformation, adapting spherical coordinates to any two points on the sphere like the two minima of the scalar 2-curvature on axisymmetric trapped surfaces.
22 pages, 5 figures
References in corpus (21)
- Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole
- Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing
- High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
- Binary black hole merger dynamics and waveforms
- Recoil velocities from equal-mass binary black-hole mergers: a systematic investigation of spin-orbit aligned configurations
- Spin Flips and Precession in Black-Hole-Binary Mergers
- Binary-black-hole initial data with nearly-extremal spins
- Fully General Relativistic Simulations of Black Hole-Neutron Star Mergers
- High-spin binary black hole mergers
- The final mass and spin of black hole mergers
- Evolving black hole-neutron star binaries in general relativity using pseudospectral and finite difference methods
- The final spin from the coalescence of aligned-spin black-hole binaries
- Circular orbits and spin in black-hole initial data
- Challenging the paradigm of singularity excision in gravitational collapse
- Binary Black Holes: Spin Dynamics and Gravitational Recoil
- Spin-orbit interactions in black-hole binaries
- Merger of black hole-neutron star binaries: nonspinning black hole case
- Approximate Killing Vectors on S^2
- The spin expansion for binary black hole merger: new predictions and future directions
- Collapse of differentially rotating supermassive stars: Post black hole formation
- Excised black hole spacetimes: quasi-local horizon formalism applied to the Kerr example
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