Numerical simulations of compact object binaries
arXiv:1203.5166 · doi:10.1088/0264-9381/29/12/124004
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.
Minor corrections, including typos and grammar
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