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20222025
most citedCircular Polarization of the Astrophysical Gravitational Wave Background

29 citations · 62 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2025★ 1 cited

Inferring cosmological parameters from galaxy and dark sirens cross-correlation

Giona Sala, Alessandro Cuoco, Julien Lesgourgues +3

The number of observed gravitational wave (GW) events is growing fast thanks to rapidly improving detector sensitivities. GWs from compact binary coalescences like Black Holes or N…

astro-ph.CO2024

Inflationary Initial Conditions for the Cosmological Gravitational Wave Background

Lorenzo Valbusa Dall'Armi, Alina Mierna, Sabino Matarrese +1

The initial conditions on the anisotropies of the stochastic gravitational-wave background of cosmological origin (CGWB) largely depend on the mechanism that generates the gravitat…

astro-ph.CO2024★ 4 cited

Gravitational wave background from primordial black holes in globular clusters

Eleonora Vanzan, Sarah Libanore, Lorenzo Valbusa Dall'Armi +2

Primordial black holes still represent a viable candidate for a significant fraction, if not for the totality, of dark matter. If these compact objects have masses of order tens of…

gr-qc2023★ 2 cited

GW_CLASS: Cosmological Gravitational Wave Background in the Cosmic Linear Anisotropy Solving System

Florian Schulze, Lorenzo Valbusa Dall'Armi, Julien Lesgourgues +5

The anisotropies of the Cosmological Gravitational Wave Background (CGWB) retain information about the primordial mechanisms that source the gravitational waves and about the geome…

astro-ph.CO2023★ 29 cited

Circular Polarization of the Astrophysical Gravitational Wave Background

Lorenzo Valbusa Dall'Armi, Atsushi Nishizawa, Angelo Ricciardone +1

The circular polarization of gravitational waves is a powerful observable to test parity violation in gravity and to distinguish between the primordial or the astrophysical origin…

astro-ph.CO2022★ 26 cited

The Dipole of the Astrophysical Gravitational-Wave Background

Lorenzo Valbusa Dall'Armi, Angelo Ricciardone, Daniele Bertacca

One of the main pillars of the ΛCDM model is the Cosmological Principle, which states that our Universe is statistically isotropic and homogeneous on large scales. Here we test thi…