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      Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms

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          Physics, Astrophysics and Cosmology with Gravitational Waves

          Gravitational wave detectors are already operating at interesting sensitivity levels, and they have an upgrade path that should result in secure detections by 2014. We review the physics of gravitational waves, how they interact with detectors (bars and interferometers), and how these detectors operate. We study the most likely sources of gravitational waves and review the data analysis methods that are used to extract their signals from detector noise. Then we consider the consequences of gravitational wave detections and observations for physics, astrophysics, and cosmology.
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            Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries

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              Calibration of moving puncture simulations

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                Author and article information

                Journal
                PRLTAO
                Physical Review Letters
                Phys. Rev. Lett.
                American Physical Society (APS)
                0031-9007
                1079-7114
                October 2014
                October 2014
                : 113
                : 15
                Article
                10.1103/PhysRevLett.113.151101
                4498519d-8b95-46b8-93ff-3dce4a9fb761
                © 2014

                http://link.aps.org/licenses/aps-default-license

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