activity
20232026
most citedEfficient multi-timescale dynamics of precessing black-hole binaries

27 citations · 104 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

The accuracy of merger times in hierarchical black hole triples

Giulia Fumagalli, Alejandro Vigna-Gómez

Orbit-averaged equations are widely used to model the gravitational-wave-driven evolution of compact binaries. Their validity relies on the radiation-reaction timescale being much…

gr-qc2025

Coincident morphological transitions in precessing black-hole binaries

Davide Gerosa, Giulia Foroni, Giulia Fumagalli +1

We present new insights into the phenomenology of post-Newtonian spin precession in black-hole binaries. Using multi-timescale methods, previous work has shown that the precession…

gr-qc2025

PRECESSION 2.1: black-hole binary spin precession on eccentric orbits

Giulia Fumagalli, Davide Gerosa, Nicholas Loutrel

We present version 2.1 of the public code {\sc precession}, a Python module for studying the post-Newtonian dynamics of precessing black hole binaries. In this release, we extend t…

astro-ph.HE2025★ 6 cited

Distinguishing the Origin of Eccentric Black Hole Mergers with Gravitational-wave Spin Measurements

Jakob Stegmann, Davide Gerosa, Isobel Romero-Shaw +3

It remains an open question whether the binary black hole mergers observed with gravitational-wave detectors originate from the evolution of isolated massive binary stars or were d…

gr-qc2025★ 8 cited

Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory

Giulia Fumagalli, Nicholas Loutrel, Davide Gerosa +1

Eccentric black-hole binaries are among the most awaited sources of gravitational waves, yet their dynamics lack a consistent framework that provides a detailed and physically robu…

gr-qc2024★ 20 cited

Orbital eccentricity in general relativity from catastrophe theory

Matteo Boschini, Nicholas Loutrel, Davide Gerosa +1

While the orbital eccentricity is a key feature of the gravitational two-body problem, providing an unambiguous definition in general relativity poses significant challenges. Despi…

astro-ph.HE2024★ 22 cited

Residual eccentricity as a systematic uncertainty on the formation channels of binary black holes

Giulia Fumagalli, Isobel Romero-Shaw, Davide Gerosa +3

Resolving the formation channel(s) of merging binary black holes is a key goal in gravitational-wave astronomy. The orbital eccentricity is believed to be a precious tracer of the…

astro-ph.HE2023★ 1 cited

The impact of outliers on pulsar timing arrays

Giulia Fumagalli, Golam Shaifullah, Alberto Sesana

The detection of gravitational waves with Pulsar Timing Arrays (PTAs) requires precise measurement of the difference between the pulsars' timing models and their observed pulses, a…

gr-qc2023★ 20 cited

Spin-eccentricity interplay in merging binary black holes

Giulia Fumagalli, Davide Gerosa

Orbital eccentricity and spin precession are precious observables to infer the formation history of binary black holes with gravitational-wave data. We present a post-Newtonian, mu…

gr-qc2023★ 27 cited

Efficient multi-timescale dynamics of precessing black-hole binaries

Davide Gerosa, Giulia Fumagalli, Matthew Mould +4

We present analytical and numerical progress on black-hole binary spin precession at second post-Newtonian order using multi-timescale methods. In addition to the commonly used eff…