Perturbative effects of spinning black holes with applications to recoil velocities
arXiv:1011.2767 · doi:10.1088/0264-9381/28/13/134005
Abstract
Recently, we proposed an enhancement of the Regge-Wheeler-Zerilli formalism for first-order perturbations about a Schwarzschild background that includes first-order corrections due to the background black-hole spin. Using this formalism, we investigate gravitational wave recoil effects from a spinning black-hole binary system analytically. This allows us to better understand the origin of the large recoils observed in full numerical simulation of spinning black hole binaries.
arXiv commentProceedings of Theory Meets Data Analysis at Comparable and Extreme Mass Ratios (NRDA/Capra 2010), Perimeter Institute, June 2010 - 12 pages
References in corpus (22)
- Evolution of Binary Black Hole Spacetimes
- Accurate Evolutions of Orbiting Black-Hole Binaries Without Excision
- Gravitational wave extraction from an inspiraling configuration of merging black holes
- Coalescing binary systems of compact objects to (post)$^{5/2}-Newtonian order. V. Spin Effects
- Large Merger Recoils and Spin Flips From Generic Black-Hole Binaries
- Maximum gravitational recoil
- Analytic black hole perturbation approach to gravitational radiation
- Remnant Masses, Spins and Recoils from the Merger of Generic Black-Hole Binaries
- Gravitational field and equations of motion of spinning compact binaries to 2.5 post-Newtonian order
- Further insight into gravitational recoil
- Orbital Evolution of Extreme-Mass-Ratio Black-Hole Binaries with Numerical Relativity
- Second Order Quasi-Normal Mode of the Schwarzschild Black Hole
- Intermediate-mass-ratio black hole binaries: intertwining numerical and perturbative techniques
- Modeling gravitational recoil from precessing highly-spinning unequal-mass black-hole binaries
- Low multipole contributions to the gravitational self-force
- Recoil velocity at 2PN order for spinning black hole binaries
- Binary black hole merger gravitational waves and recoil in the large mass ratio limit
- Intermediate Mass Ratio Black Hole Binaries: Numerical Relativity meets Perturbation Theory
- Momentum flow in black-hole binaries: II. Numerical simulations of equal-mass, head-on mergers with antiparallel spins
- Gravitational Radiation from Plunging Orbits - Perturbative Study -
- Regular second order perturbations of binary black holes: The extreme mass ratio regime
- The collision of two slowly rotating, initially non boosted, black holes in the close limit
Cited by in corpus (5)
- Remnant mass, spin, and recoil from spin aligned black-hole binaries
- Nonlinear Gravitational Recoil from the Mergers of Precessing Black-Hole Binaries
- Modeling the remnant mass, spin, and recoil from unequal-mass, precessing black-hole binaries: The Intermediate Mass Ratio Regime
- A note on gravitational wave extraction from binary simulations
- Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications