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An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
Alejandro Bohé, Lijing Shao, Andrea Taracchini +17
We improve the accuracy of the effective-one-body (EOB) waveforms that were employed during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing black h…
Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian
Jan Steinhoff, Tanja Hinderer, Alessandra Buonanno +1
Tidal effects have an important impact on the late inspiral of compact binary systems containing neutron stars. Most current models of tidal deformations of neutron stars assume th…
Validating the effective-one-body model of spinning, precessing binary black holes against numerical relativity
Stanislav Babak, Andrea Taracchini, Alessandra Buonanno
In Ref. [1], the properties of the first gravitational wave detected by LIGO, GW150914, were measured by employing an effective-one-body (EOB) model of precessing binary black hole…
Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach
Tanja Hinderer, Andrea Taracchini, Francois Foucart +11
Extracting the unique information on ultradense nuclear matter from the gravitational waves emitted by merging, neutron-star binaries requires robust theoretical models of the sign…