activity
20192021
most citedThe properties of merging black holes and neutron stars across cosmic time

141 citations · 238 across the 2 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2025

A new prescription for the spectral properties of population III stellar populations

Marie Lecroq, Stéphane Charlot, Alessandro Bressan +7

We investigated various emission properties of extremely low metallicity stellar populations in the Epoch of Reionization (EoR), using the new GALSEVN model, which has shown promis…

astro-ph.GA2021

Dynamics of binary black holes in low-mass young star clusters

Sara Rastello, Michela Mapelli, Ugo N. di Carlo +5

Young star clusters are dynamically active stellar systems and are a common birthplace for massive stars. Low-mass star clusters ( M) are more numerous than…

astro-ph.HE2021

GW190521 formation via three-body encounters in young massive star clusters

Marco Dall'Amico, Michela Mapelli, Ugo N. Di Carlo +5

GW190521 is the most massive binary black hole (BBH) merger observed to date, and its primary component lies in the pair-instability (PI) mass gap. Here, we investigate the formati…

astro-ph.HE2021

Hierarchical black hole mergers in young, globular and nuclear star clusters: the effect of metallicity, spin and cluster properties

Michela Mapelli, Marco Dall'Amico, Yann Bouffanais +8

We explore hierarchical black hole (BH) mergers in nuclear star clusters (NSCs), globular clusters (GCs) and young star clusters (YSCs), accounting for both original and dynamicall…

astro-ph.HE2020

The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution

Filippo Santoliquido, Michela Mapelli, Nicola Giacobbo +2

We evaluate the redshift distribution of binary black hole (BBH), black hole - neutron star binary (BHNS) and binary neutron star (BNS) mergers, exploring the main sources of uncer…

astro-ph.HE2020

The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries

Filippo Santoliquido, Michela Mapelli, Yann Bouffanais +5

Next generation ground-based gravitational-wave detectors will observe binary black hole (BBH) mergers up to redshift , probing the evolution of compact binary (CB) m…