The collision of boosted black holes
arXiv:gr-qc/9608064 · doi:10.1103/PhysRevD.55.829
Abstract
We study the radiation from a collision of black holes with equal and opposite linear momenta. Results are presented from a full numerical relativity treatment and are compared with the results from a ``close-slow'' approximation. The agreement is remarkable, and suggests several insights about the generation of gravitational radiation in black hole collisions.
8 pages, RevTeX, 3 figures included with epsf
References in corpus (2)
Cited by in corpus (45)
- Measuring gravitational waves from binary black hole coalescences: I. Signal to noise for inspiral, merger, and ringdown
- Toward faithful templates for non-spinning binary black holes using the effective-one-body approach
- Numerical Relativity: A review
- Estimating the final spin of a binary black hole coalescence
- The high-energy collision of two black holes
- Modeling gravitational radiation from coalescing binary black holes
- Black-hole hair loss: learning about binary progenitors from ringdown signals
- Gauge invariant perturbations of Schwarzschild black holes in horizon-penetrating coordinates
- Nonexistence of conformally flat slices of the Kerr spacetime
- Mode coupling in the nonlinear response of black holes
- Understanding initial data for black hole collisions
- The numerical relativity breakthrough for binary black holes
- Head--on Collision of Two Unequal Mass Black Holes
- An Axisymmetric Gravitational Collapse Code
- Evolving the Bowen-York initial data for spinning black holes
- What we (don't) know about black hole formation in high-energy collisions
- 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
- Inspiralling black holes: the close limit
- Head-on collision of unequal mass black holes: close-limit predictions
- The collision of boosted black holes: second order close limit calculations
- Gauge invariant formalism for second order perturbations of Schwarzschild spacetimes
- Close-limit analysis for head-on collision of two black holes in higher dimensions: Brill-Lindquist initial data
- Three Dimensional Distorted Black Holes
- Initial data for superposed rotating black holes
- Close-slow analysis for head-on collision of two black holes in higher dimensions: Bowen-York initial data
- Close limit of grazing black hole collisions: non-spinning holes
- Gravitational bremsstrahlung in ultra-planckian collisions
- The imposition of Cauchy data to the Teukolsky equation I: The nonrotating case
- Adaptive computation of gravitational waves from black hole interactions
- A New Method for Solving the Initial Value Problem with Application to Multiple Black Holes
- Formation of a rotating hole from a close limit head-on collision
- Perturbative evolution of conformally flat initial data for a single boosted black hole
- Blue spectra and induced formation of primordial black holes
- Collision of spinning black holes in the close limit
- Close limit evolution of Kerr-Schild type initial data for binary black holes
- Regularization of the Teukolsky Equation for Rotating Black Holes
- Quasi-spherical approximation for rotating black holes
- Applications of the close-limit approximation: horizonless compact objects and scalar fields
- Collision of spinning black holes in the close limit: The parallel spin case
- The two-phase approximation for black hole collisions: Is it robust?
- Estimating the Final Spin of Binary Black Holes Merger in STU Supergravity
- Gravitational radiation sources and signatures
- Challenging theories of gravitation: dark matter, compact objects and gravitational waves
- Comparing numerical relativity and perturbation theory waveforms for a non-spinning equal-mass binary