1 code implementation • 27 May 2014 • M. Dominik, E. Berti, R. O'Shaughnessy, I. Mandel, K. Belczynski, C. Fryer, D. Holz, T. Bulik, F. Pannarale
The unprecedented range of second-generation gravitational-wave (GW) observatories calls for refining the predictions of potential sources and detection rates.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
