Mourier, Pierre; Jiménez Forteza, Xisco; Pook-Kolb, Daniel; Krishnan, Badri; Schnetter, Erik
(Ridge, NY : American Physical Society, 2021)
It is expected that all astrophysical black holes in equilibrium are well described by the Kerr solution. Moreover, any black hole far away from equilibrium, such as one initially formed in a compact binary merger or by ...