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Binary black hole coalescence in the extreme-mass-ratio limit: testing and improving the effective-one-body multipolar waveform
Sebastiano Bernuzzi, Alessandro Nagar, Anil Zenginoglu
We discuss the properties of the effective-one-body (EOB) multipolar gravitational waveform emitted by nonspinning black-hole binaries of masses and in the extreme-mass-rat…
Analytic modelling of tidal effects in the relativistic inspiral of binary neutron stars
Luca Baiotti, Thibault Damour, Bruno Giacomazzo +2
To detect the gravitational-wave (GW) signal from binary neutron stars and extract information about the equation of state of matter at nuclear density, it is necessary to match th…
Binary black hole merger in the extreme-mass-ratio limit: a multipolar analysis
Sebastiano Bernuzzi, Alessandro Nagar
Building up on previous work, we present a new calculation of the gravitational wave (GW) emission generated during the transition from quasi-circular inspiral to plunge, merger an…