Ultimate Black Hole Recoil: What the maximum high energy collisions kick is?

Fuente: arXiv
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Main Authors: Healy, James, Lousto, Carlos O.
Format: Preprint
Published: 2022
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author Healy, James
Lousto, Carlos O.
author_facet Healy, James
Lousto, Carlos O.
contents We performed a series of 1381 full numerical simulations of high energy collision of black holes to search for the maximum recoil velocity after their merger. We consider equal mass binaries with opposite spins pointing along their orbital plane and perform a search of spin orientations, impact parameters, and initial linear momenta to find the maximum recoil for a given spin magnitude $s$. This spin sequence for $s=0.4, 0.7, 0.8, 0.85, 0.9$ is then extrapolated to the extreme case, $s=1$, to obtain an estimated maximum recoil velocity of $28,562\pm 342$ km/s, thus approximately bounded by $10\%$ the speed of light.
format Preprint
id arxiv_https___arxiv_org_abs_2301_00018
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle Ultimate Black Hole Recoil: What the maximum high energy collisions kick is?
Healy, James
Lousto, Carlos O.
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Theory
We performed a series of 1381 full numerical simulations of high energy collision of black holes to search for the maximum recoil velocity after their merger. We consider equal mass binaries with opposite spins pointing along their orbital plane and perform a search of spin orientations, impact parameters, and initial linear momenta to find the maximum recoil for a given spin magnitude $s$. This spin sequence for $s=0.4, 0.7, 0.8, 0.85, 0.9$ is then extrapolated to the extreme case, $s=1$, to obtain an estimated maximum recoil velocity of $28,562\pm 342$ km/s, thus approximately bounded by $10\%$ the speed of light.
title Ultimate Black Hole Recoil: What the maximum high energy collisions kick is?
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Theory
url https://arxiv.org/abs/2301.00018