no code implementations • 4 Mar 2020 • Matthew Mould, Davide Gerosa
We finally apply these findings to a simple astrophysical population of binary black holes where a formation mechanism aligns the spins without preference for co- or counter-alignment, as might be the case for stellar-mass black holes embedded in the accretion disk of a supermassive black hole.
General Relativity and Quantum Cosmology Astrophysics of Galaxies High Energy Astrophysical Phenomena
