activity
20172022
most citedEccentricity evolution of massive black hole binaries from formation to coalescence

52 citations · 267 across the 8 of their papers we have counts for

collaborators

17 papers

astro-ph.GA20221 cited

Disc instability and bar formation: view from the IllustrisTNG simulations

David Izquierdo-Villalba, Silvia Bonoli, Yetli Rosas-Guevara +7

We make use of z = 0 samples of strongly barred and unbarred disc galaxies from the TNG100 and TNG50 cosmological hydrodynamical simulations to assess the performance of the simple…

astro-ph.GA202252 cited

Eccentricity evolution of massive black hole binaries from formation to coalescence

Alessia Gualandris, Fazeel Mahmood Khan, Elisa Bortolas +4

Coalescing supermassive black hole binaries (BHBs) are expected to be the loudest sources of gravitational waves (GWs) in the Universe. Detection rates for ground or space-based de…

astro-ph.HE202139 cited

The competing effect of gas and stars in massive black hole binaries evolution

Elisa Bortolas, Alessia Franchini, Matteo Bonetti +1

Massive black hole binaries are predicted to form during the hierarchical assembly of cosmic structures and will represent the loudest sources of low-frequency gravitational waves…

astro-ph.HE2021

Binary black hole signatures in polarized light curves

Massimo Dotti, Matteo Bonetti, Daniel J. D'Orazio +2

Variable active galactic nuclei showing periodic light curves have been proposed as massive black hole binary (MBHB) candidates. In such scenarios the periodicity can be due to rel…

astro-ph.GA202043 cited

Unveiling early black hole growth with multi-frequency gravitational wave observations

Rosa Valiante, Monica Colpi, Raffaella Schneider +7

Third Generation ground based Gravitational Wave Interferometers, like the Einstein Telescope (ET), Cosmic Explorer (CE), and the Laser Interferometer Space Antenna (LISA) will det…

astro-ph.GA2020

Dynamical evolution of massive perturbers in realistic multi-component galaxy models I: implementation and validation

Matteo Bonetti, Elisa Bortolas, Alessandro Lupi +1

Galaxies are self-gravitating structures composed by several components encompassing spherical, axial and triaxial symmetry. Although real systems feature heterogeneous components…