activity
20142026
most citedMerging black hole binaries with the SEVN code

273 citations · 1.4k across the 71 of their papers we have counts for

collaborators

74 papers

astro-ph.GA2026

A triple-induced merger in T Ori C, solves the proplyd lifetime problem and the curiously young shell of M42

Maite Wilhelm, Alessandro Alberto Trani, Simon Portegies Zwart

There has long been a tension between the stellar ages in the Orion Nebula Cluster and the rapid external photoevaporation of its protoplanetary discs. Recently, the shell of the O…

astro-ph.EP2026

Planar Three-Body Problem: theoretical predictions and simulation results

Yogesh Dandekar, Ethan Springer, Shoval Zard +3

We investigate the statistical properties of the non-hierarchical planar three-body problem, relevant to astrophysical systems with nearly planar dynamics, including protoplanetary…

astro-ph.GA2026

On an empirical method to build near-equilibrium axisymmetric and triaxial galaxy models

Pierfrancesco Di Cintio, Alessandro Alberto Trani, Valentina Cesare

We introduce a numerical technique to implement body realizations of axisymmetric and triaxial self-gravitating system starting from a spherical self-consistent models for whic…

astro-ph.GA2026

AGN-driven BBH mergers: Black hole populations and hierarchical growth across the AGN parameter space

Maria Paola Vaccaro, Michela Mapelli, Alessandro Alberto Trani +1

Active galactic nuclei (AGNs) have been proposed as efficient environments for the formation of binary black holes (BBHs). We present an updated semi-analytical framework for BBH f…

astro-ph.SR2026

The impact of envelope binding energies on the merger rate density of binary compact objects

Cecilia Sgalletta, Guglielmo Costa, Giuliano Iorio +8

The common envelope (CE) phase plays a key role in the formation of binary compact object systems. Its final outcome strongly depends on the envelope binding energy, but this quant…

astro-ph.IM2026

A benchmark for binary star interaction with a supermassive black hole in general relativity

Megha Sharma, Alexander Heger, Daniel J. Price +4

Most galaxies have supermassive black holes (SMBH) at their centres, surrounded by stars with binary systems also present in this environment. We use two schemes - post-Newtonian (…