collaborators

9 papers

astro-ph.HE2026

Shaping binary black hole merger efficiency with gravitational wave observations

Michele Bosi, Lumen Boco, Stefano Torniamenti +5

Gravitational wave (GW) astronomy offers unprecedented insights into binary black hole (BBH) coalescence. However, many of the key quantities involved remain inaccessible to direct…

astro-ph.GA2026

StAGE: Stellar Archaeology-driven Galaxy Evolution II. Binary Black Hole Mergers in Quiescent Galaxies and their Star-forming Progenitors

Irene Iorio, Andrea Lapi, Lumen Boco +5

We apply StAGE, a data-driven galaxy-evolution framework based on stellar archaeology, to study binary black hole (BBH) mergers in quiescent galaxies (QGs) and their star-forming p…

gr-qc2026

Breaking binary formation mechanism degeneracies with gravitational wave clustering

Nicola Bellomo, Michele Bosi, Sarah Libanore +4

Thanks to the almost 400 gravitational wave events detected, we are currently able to grasp the fundamental features of black hole mass, spin, and distance distributions. However,…

astro-ph.HE2026

A binary black hole merger rate comparison within the same metallicity-star formation rate framework

Lumen Boco, Michele Bosi, Cecilia Sgalletta +2

Recent studies have suggested that binary population synthesis models, when coupled with observationally based, metallicity-dependent SFRD, overpredict the observed local BBH merge…

astro-ph.CO2026

Using SKAO to Understand the Clustering of Gravitational Wave Sources

Michele Bosi, Sarah Libanore, Nicola Bellomo +4

Coalescing Binary Black Holes (BBHs) trace the Large-Scale Structure (LSS) of the Universe, and their clustering properties can be extracted from Gravitational Wave (GW) data. Next…

astro-ph.HE2026

Can current models predict the local black hole merger rate?

Lumen Boco, Michele Bosi, Cecilia Sgalletta +2

After four observational runs, the Ligo-Virgo-Kagra collaboration estimated a local binary black hole (BBH) merger rate density of $R_{0,\textrm{LVK}}\simeq 14-26\,\textrm{Gpc}^{-3…

astro-ph.CO2025

Cosmography via stellar archaeology of low-redshift early-type galaxies from SDSS

Carlos A. Álvarez, Marcos M. Cueli, Alessandro Bressan +5

Cosmic chronometers offer a model-independent way to trace the expansion history of the Universe via the dating of passively evolving objects. This enables testing the validity of…

astro-ph.CO2025

Semi-empirical Framework of Supermassive Black Hole Evolution: Highlighting a possible tension between Demographics and Gravitational Wave Background

Andrea Lapi, Francesco Shankar, Michele Bosi +4

The evolution of the supermassive Black Hole (BH) population across cosmic times remains a central unresolved issue in modern astrophysics, due to the many noticeable uncertainties…

astro-ph.GA2025

StAGE: Stellar Archaeology-driven Galaxy Evolution

Michele Bosi, Andrea Lapi, Lumen Boco +10

We build a semi-empirical framework of galaxy evolution (dubbed StAGE) firmly grounded on stellar archaeology. The latter provides data-driven prescriptions that, on a population s…