Confusion noise from astrophysical backgrounds at third-generation gravitational-wave detector networks
We compute the impact of astrophysical “confusion noise” in the search for cosmological gravitational-wave backgrounds
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We compute the impact of astrophysical “confusion noise” in the search for cosmological gravitational-wave backgrounds
We derive the spectral density of the stochastic gravitational-wave background generated by compact binary coalescences
We examine the scientific potential of a European third-generation network comprising two L-shaped detectors, one underground and one on-surface
We develop a Fisher tool for forecasts on population analyses at third-generation detectors
We study the prospects of classifying binary black holes originating from Population III stars observed through gravitational waves at the Einstein Telescope using machine learning
We investigate the prospects of observing electromagnetic counterparts to black hole-neutron star mergers detected through gravitational waves during O4 and O5
We develop a way to perform unbiased estimations of the expansion rate of the Universe from gravitational-wave + γ-ray burst detections and a new gravitational-wave likelihood approximant
We provide a first comprehensive analysis of the Lunar Gravitational-wave Antenna science case including its multi-messenger aspects and lunar science
We develop a code to perform a joint population and cosmological inference on gravitational-wave data and galaxy catalogs, and apply it to simulated O4 and O5 catalogs of gravitational waves
We study how binary neutron star mergers observations at the Einstein Telescope can improve our understanding of their equation of state
We analyze in detail the impact of different designs for the Einstein Telescope on our future capability of observing key quantities characterizing primordial black hole mergers and also perform a population analysis.
We examine the scientific perspectives of different designs for the Einstein Telescope, with a detailed evaluation of the science case.
We provide useful metrics to assess the capabilities of third-generation gravitational-wave detectors in the observation of high-redshift sources.
Prospects of combining γ-ray burst polarization measurements and gravitational-wave observations to extract information on the γ-ray bursts emission model.
Up-to-date forecasts of the capabilities of Einstein Telescope and Cosmic Explorer to observe compact binary mergers.
We release, review, and validate the GWFAST code!
We show how the narrowness of the binary neutron star mass distribution can give clear signatures of modified gravity.
We show how quadruply lensed gravitational-wave events can be an extremely valuable candidate to constrain modifications of GR at cosmological scales.
We exploit gravitational-wave detections and a galaxy catalog to obtain constraints on the expansion rate of the Universe and possible deviations from GR at cosmological scales. A public code is also released!