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Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
Isobel M. Romero-Shaw, Davide Gerosa, Nicholas Loutrel
Eccentricity and spin precession are key observables in gravitational-wave astronomy, encoding precious information about the astrophysical formation of compact binaries together w…
The Bardeen-Petterson effect, disk breaking, and the spin orientations of supermassive black-hole binaries
Nathan Steinle, Davide Gerosa
Supermassive black-hole binaries are driven to merger by dynamical friction, loss-cone scattering of individual stars, disk migration, and gravitational-wave emission. Two main for…
Characterization of merging black holes with two precessing spins
Viola De Renzis, Davide Gerosa, Geraint Pratten +2
Spin precession in merging black-hole binaries is a treasure trove for both astrophysics and fundamental physics. There are now well-established strategies to infer from gravitatio…
New Horizons for Fundamental Physics with LISA
K. G. Arun, Enis Belgacem, Robert Benkel +138
The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the fundamental theory of nature at play in the extreme gravity regime, where the gravitatio…
Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
Matthew Mould, Davide Gerosa, Floor S. Broekgaarden +1
Population inference of gravitational-wave catalogues is a useful tool to translate observations of black-hole mergers into constraints on compact-binary formation. Different forma…
The last three years: multiband gravitational-wave observations of stellar-mass binary black holes
Antoine Klein, Geraint Pratten, Riccardo Buscicchio +10
Understanding the formation and evolution of the stellar-mass binary black holes discovered by LIGO and Virgo is a challenge that spans many areas of astrophysics, from stellar evo…