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

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

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Showing astro-ph.GAShow all

5 papers · 1 filter

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.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.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…

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…