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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 . This spin sequence for is then extrapolated to the extreme case, , to obtain an estimated maximum recoil velocity of km/s, thus approximately bounded by the speed of light.

生成讲解博客的中文版本

生成AI智能校验的中文版本