activity
20212026
most citedScience with the Einstein Telescope: a comparison of different designs

402 citations · 566 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.IM2026

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

Ulyana Dupletsa, Francesco Iacovelli, Mikhail Korobko +23

We investigate the relationship between instrumental requirements and the scientific performance of the Einstein Telescope (ET), a third-generation (3G) gravitational-wave (GW) obs…

gr-qc2026

Cosmology and modified GW propagation from the BNS mass function at third-generation detector networks

Dounia Nanadoumgar-Lacroze, Niccolò Muttoni, Michele Maggiore +1

We perform forecasts for the Hubble parameter H_0 and for the parameter Xi_0 that describes modified gravitational-wave propagation, using information from the binary neutron star…

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

gr-qc2024

Confusion noise from astrophysical backgrounds at third-generation gravitational-wave detector networks

Enis Belgacem, Francesco Iacovelli, Michele Maggiore +2

At third-generation (3G) gravitational-wave detector networks, compact binaries coalescences produce a ``confusion noise'' due to unresolved sources and to the error in the reconst…

gr-qc2024

Comparison of global networks of third-generation gravitational-wave detectors

Michele Maggiore, Francesco Iacovelli, Enis Belgacem +2

We study the performances of a world-wide network made by a European third-generation gravitational-wave (GW) detector, together with a 40km Cosmic Explorer detector in the US, con…

gr-qc2024

The spectral density of astrophysical stochastic backgrounds

Enis Belgacem, Francesco Iacovelli, Michele Maggiore +2

We provide a detailed derivation of the spectral density of the stochastic background generated by the superposition of coalescing compact binaries. We show how the expression ofte…

gr-qc2024

Combining underground and on-surface third-generation gravitational-wave interferometers

Francesco Iacovelli, Enis Belgacem, Michele Maggiore +2

Recently, detailed studies have been made to compare the performance of the European next generation GW observatory Einstein Telescope (ET) in a single-site triangular configuratio…

astro-ph.HE2024

Accurate Standard Siren Cosmology with Joint Gravitational-Wave and -Ray Burst Observations

Michele Mancarella, Francesco Iacovelli, Stefano Foffa +2

Joint gravitational-wave (GW) and -ray burst (GRB) observations are among the best prospects for standard siren cosmology. However, the strong selection effect for the coinciden…

gr-qc2024★ 39 cited

The Lunar Gravitational-wave Antenna: Mission Studies and Science Case

Parameswaran Ajith, Pau Amaro Seoane, Manuel Arca Sedda +83

The Lunar Gravitational-wave Antenna (LGWA) is a proposed array of next-generation inertial sensors to monitor the response of the Moon to gravitational waves (GWs). Given the size…

gr-qc2023★ 402 cited

Science with the Einstein Telescope: a comparison of different designs

Marica Branchesi, Michele Maggiore, David Alonso +73

The Einstein Telescope (ET), the European project for a third-generation gravitational-wave detector, has a reference configuration based on a triangular shape consisting of three…

astro-ph.CO2023★ 3 cited

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…

astro-ph.CO2021★ 25 cited

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…