359 citations · 865 across the 22 of their papers we have counts for
13 papers · 1 filter
Reconstructing stochastic gravitational-wave signals from flavour deconstruction with LISA
Noemi Fabri, Raphael Bertrand-Delgado, Danny Laghi +1
We investigate the reconstruction of a stochastic gravitational-wave background generated by a first-order phase transition in flavour-deconstruction models using the Laser Interfe…
Reducing cosmological degeneracies by combining multiple classes of LISA gravitational-wave standard sirens
Danny Laghi, Nicola Tamanini, Alberto Sesana +6
We present the first joint gravitational-wave cosmological inference with LISA extreme mass-ratio inspirals at (galaxy redshifts) and massive black hole binaries at $z…
Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
Isaac McMahon, Danny Laghi, Marcelle Soares-Santos +9
Gravitational wave (GW) standard sirens enable independent measurements of the Hubble constant . In the absence of electromagnetic counterparts, the 'dark siren' method statis…
First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
Felipe Andrade-Oliveira, David Sanchez-Cid, Danny Laghi +1
We present a new measurement of the Hubble constant () resulting from the first joint analysis of standard sirens with weak gravitational lensing and galaxy clustering observa…
LISA Definition Study Report
Monica Colpi, Karsten Danzmann, Martin Hewitson +108
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves…
Probing modified gravitational-wave propagation with extreme mass-ratio inspirals
Chang Liu, Danny Laghi, Nicola Tamanini
Extreme mass-ratio inspirals (EMRIs), namely binary systems composed of a massive black hole and a compact stellar-mass object, are anticipated to be among the gravitational wave (…
ICAROGW: A python package for inference of astrophysical population properties of noisy, heterogeneous and incomplete observations
Simone Mastrogiovanni, Grégoire Pierra, Stéphane Perriès +6
We present icarogw 2.0, a pure CPU/GPU python code developed to infer astrophysical and cosmological population properties of noisy, heterogeneous, and incomplete observations. ica…
A novel approach to infer population and cosmological properties with gravitational waves standard sirens and galaxy surveys
Simone Mastrogiovanni, Danny Laghi, Rachel Gray +7
Gravitational wave (GW) sources at cosmological distances can be used to probe the expansion rate of the Universe. GWs directly provide a distance estimation of the source but no d…
Dark siren cosmology with binary black holes in the era of third-generation gravitational wave detectors
Niccolò Muttoni, Danny Laghi, Nicola Tamanini +2
Third-generation (3G) gravitational wave detectors, in particular Einstein Telescope (ET) and Cosmic Explorer (CE), will explore unprecedented cosmic volumes in search for compact…
Cosmology with the Laser Interferometer Space Antenna
Pierre Auclair, David Bacon, Tessa Baker +177
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravita…
Multiband gravitational wave cosmology with stellar origin black hole binaries
Niccolò Muttoni, Alberto Mangiagli, Alberto Sesana +4
Massive stellar origin black hole binaries (SBHBs), originating from stars above the pair-instability mass gap, are primary candidates for multiband gravitational wave (GW) observa…
Gravitational wave cosmology with EMRIs
Danny Laghi
We show that the loudest extreme mass-ratio inspirals (EMRIs) detected by the future space-based gravitational wave detector LISA can be used as dark standard sirens, statistically…
Gravitational wave cosmology with extreme mass-ratio inspirals
Danny Laghi, Nicola Tamanini, Walter Del Pozzo +4
The Laser Interferometer Space Antenna (LISA) will open the mHz frequency window of the gravitational wave (GW) landscape. Among all the new GW sources expected to emit in this fre…