Year: 2012
Type: article
Abstract: Coalescing compact object binaries consisting of black holes and/or neutron stars are a prime target for ground-based gravitational wave detectors. This paper reviews the status of numerical simulations of these systems with an emphasis on recent progress.
Source: Classical and Quantum Gravity
Author: Harald P Pfeiffer
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2036940811
