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Perturbative effects of spinning black holes with applications to recoil velocities
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Perturbative effects of spinning black holes with applications to recoil velocities
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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.
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Cited by 1 Pith paper
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Recoil kicks from binary black hole mergers in GWTC catalogs: implications for retention and hierarchical mergers
Recoil kicks are inferred for GWTC-4 binary black hole events with values up to nearly 1000 km/s for some, yielding retention probabilities of 1-5% in globular clusters and 70-100% in elliptical galaxies.
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