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Rival Families: Waveforms from Resonant Black-Hole Binaries as Probes of Their Astrophysical Formatewtonian theory predicts the existence of two one-parameter families of equilibrium solutions (“resonances”) in which the angular momentum and both spins share a common plane and precess at the same frequency. The two families are differentiated by either aligned or anti-aligned spin components in t

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Gravitational Wave Verification Sources, weak gravitational wave sources. However, there are nine systems where the gravitational wave strain is strong enough to make them verification sources for gravitational wave missions, e.g. the evolved Laser Interferometer Space Antenna (.). Here we present a summary of the physical characteristics

MEAN

The Gravitational Wave Emission of White Dwarf Dynamical Interactions, it with the sensitivity curves of planned space-borne gravitational wave detectors, like eLISA and ALIA. We find that for the three possible outcomes of these interactions—which are the formation of an eccentric binary system, a lateral collision in which several mass transfer episodes occur, and a

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Gravitational Recoil and Astrophysical Impact,tion, imparts a gravitational recoil on the emitting source. Numerical relativity simulations have revealed that this effect can lead to astonishingly large kick velocities, so-called ., of several thousand km/s in the inspiral and merger of black-hole binaries. We here discuss the calculation of th

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Extraction of GWs from a Numerical Simulation,d characteristic extraction. These methods are reviewed, and the strengths and weaknesses of each method are discussed. The accuracy of the methods is compared for astrophysical scenarios that are commonly simulated numerically.

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Quasinormal Modes Beyond Kerr,rr black holes. We discuss a method for computing the QNMs of spacetimes which are slightly deformed from Kerr. We mention two example applications: the parametric, turbulent instability of scalar fields on a background which includes a gravitational QNM, and the shifts to the QNM frequencies of Ker

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https://doi.org/10.1007/978-0-387-28745-4Currently, the best experiments supporting this hypothesis are based on high-precision timing of radio pulsars. This chapter reviews recent advances in the field with a focus on compact binary millisecond pulsars with white-dwarf (WD) companions. These systems—if modeled properly—provide an unparall