Zucker, Michael E.; Wipf, Christopher C.; Weiss, Rainer; Waldman, Samuel J.; Stein, Leo Chaim; Stein, Andrew J.; Smith, Nicolas de Mateo; Shoemaker, David H.; Shapiro, B.; Sarin, P.; Ruet, L.; Mittleman, Richard K.; Mason, Kenneth R.; Markowitz, Jared John; MacInnis, Myron E.; Katsavounidis, Erotokritos; Hughey, Brennan J.; Harry, Gregory; Grimaldi, F.; Goda, K.; Fritschel, Peter K.; Foley, Stephany; Evans, Matthew J.; Duke, I.; Donovan, Frederick J.; Corbitt, Thomas R.; Cao, Junwei; Brunet, G.; Bodiya, Timothy Paul; Blackburn, Lindy L.; Barsotti, Lisa; Mavalvala, Nergis
(American Physical Society, 2009-09)
According to general relativity a perturbed black hole will settle to a stationary configuration by the emission of gravitational radiation. Such a perturbation will occur, for example, in the coalescence of a black hole ...