Authors: Harald P. Pfeiffer
Date: 23 Mar 2012
Abstract: Coalescing compact object binaries consisting of black holes and/or Neutron stars are a prime target for ground-based gravitational wave detectors. This article reviews the status of numerical simulations of these systems, with an emphasis on recent progress.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis