activity
20232026
most citedOpportunities and limits of lunar gravitational-wave detection

15 citations · 24 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

The STARfall pathway: forging intermediate-mass black holes through stellar collisions in dense star clusters

Filippo Simonato, Manuel Arca Sedda, Taeho Ryu +15

Intermediate-mass black holes (IMBHs, ) are elusive objects bridging the gap between stellar-mass and supermassive black holes, whose o…

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…

astro-ph.HE2026

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae

Francesco Gabrielli, Cristiano Ugolini, Lavinia Paiella +12

Pair-instability supernovae (PISNe) are among the most luminous transients in the Universe. However, they have never been confidently observed. Solving this puzzle would have key i…

astro-ph.IM2026

Advanced Virgo Plus for O5 -- Design Report Overview

F. Acernese, A. Agapito, D. Agarwal +578

This document presents an overview of the design, implementation, and expected performance of the Advanced Virgo Plus (AdV+) upgrades in view of the O5 observing run. Following the…

astro-ph.GA2026

Isolated or Dynamical? Tracing Black Hole Binary Formation through the Population of Gravitational-Wave Sources

Manuel Arca Sedda, Lavinia Paiella, Cristiano Ugolini +5

The population of binary black hole (BBH) mergers observed by the LIGO-Virgo-KAGRA (LVK) collaboration offers a window into the cosmic evolution of compact binaries and their forma…

astro-ph.HE2025

Uncovering the population of compact binary mergers and their formation pathways with gravitational waves through the Einstein Telescope

M. Arca-Sedda, I. Dvorkin, G. Franciolini +19

Ground-based gravitational-wave (GW) observatories have transformed our view of compact-object mergers, yet their reach still limits a comprehensive reconstruction of the processes…

astro-ph.GA2025★ 6 cited

Seeds to success: growing heavy black holes in dense star clusters

Lavinia Paiella, Manuel Arca Sedda, Benedetta Mestichelli +1

The observational dearth of black holes (BHs) with masses between 100 and 100,000 raises questions about the nature of intermediate-mass black holes (IMBHs). Propos…

astro-ph.GA2025

Assembling GW231123 in star clusters through the combination of stellar binary evolution and hierarchical mergers

Lavinia Paiella, Cristiano Ugolini, Mario Spera +2

GW231123 is the most massive binary black hole (BBH) merger detected to date by the LIGO-Virgo-KAGRA collaboration. With at least one black hole (BH) in the upper-mass gap and both…

gr-qc2025★ 2 cited

Comparing astrophysical models to gravitational-wave data in the observable space

Alexandre Toubiana, Davide Gerosa, Matthew Mould +9

Comparing population-synthesis models to the results of hierarchical Bayesian inference in gravitational-wave astronomy requires a careful understanding of the domain of validity o…

astro-ph.GA2025★ 1 cited

Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars

Benedetta Mestichelli, Michela Mapelli, Filippo Santoliquido +9

Population III (Pop.III) stars are expected to be massive and to undergo minimal mass loss due to their lack of metals, making them ideal progenitors of black holes and neutron…

astro-ph.IM2023★ 15 cited

Opportunities and limits of lunar gravitational-wave detection

Andrea Cozzumbo, Benedetta Mestichelli, Marco Mirabile +3

A new era of lunar exploration has begun with participation of all major space agencies. This activity brings opportunities for revolutionary science experiments and observatories…