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87 papers
Spinformation: do gravitational-wave events carry information beyond effective spins?
Cailin Plunkett, Jack Heinzel, Noah E. Wolfe +2
While the spin vectors of binary black holes offer insight into the astrophysical formation channels of these systems, individual spins are less precisely measured through gravitat…
Not all spins of black-hole binaries formed in clusters are isotropic and not all spins of black-hole binaries formed in isolation are aligned
Sofia Dossena, Davide Gerosa, Tristan Bruel
Spin directions are promising observables for distinguishing between the formation channels of merging stellar-mass binary black holes with gravitational-wave observations. In this…
Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs
Matthew Mould, Christopher J. Moore, Davide Gerosa
Searching for gravitational-wave signals is a challenging and computationally intensive endeavor undertaken by multiple independent analysis pipelines. While detection depends only…
Waveform Modelling for the Laser Interferometer Space Antenna
LISA Consortium Waveform Working Group, Niayesh Afshordi, Sarp Akçay +144
LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will exp…
Spin-eccentricity interplay in merging binary black holes
Giulia Fumagalli, Davide Gerosa
Orbital eccentricity and spin precession are precious observables to infer the formation history of binary black holes with gravitational-wave data. We present a post-Newtonian, mu…
Black-hole mergers in disklike environments could explain the observed - correlation
Alessandro Santini, Davide Gerosa, Roberto Cotesta +1
Current gravitational-wave data from stellar-mass black-hole binary mergers suggest a correlation between the binary mass ratio and the effective spin : more un…