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Gravitational-Wave Astronomy with Inspiral Signals of Spinning Compact-Object Binaries
M. V. van der Sluys, C. Roever, A. Stroeer +6
Inspiral signals from binary compact objects (black holes and neutron stars) are primary targets of the ongoing searches by ground-based gravitational-wave interferometers (LIGO, V…
Spin distribution following minor mergers and the effect of spin on the detection range for low-mass-ratio inspirals
Ilya Mandel
We compute the probability distribution for the spin of a black hole following a series of minor mergers with isotropically distributed, non-spinning, inspiraling compact objects.…
Rates and Characteristics of Intermediate Mass Ratio Inspirals Detectable by Advanced LIGO
Ilya Mandel, Duncan A. Brown, Jonathan R. Gair +1
Gravitational waves (GWs) from the inspiral of a neutron star (NS) or stellar-mass black hole (BH) into an intermediate-mass black hole (IMBH) with mass between ~50 and ~350 solar…
Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA
Pau Amaro-Seoane, Jonathan R. Gair, Marc Freitag +4
Black hole binaries with extreme () or intermediate () mass ratios are among the most interesting gravitational wave sources that are expected to…