activity
20122025
most citedA Census of Young Stars and Brown Dwarfs in IC 348 and NGC 1333

117 citations · 1k across the 31 of their papers we have counts for

collaborators

31 papers

gr-qc2025★ 1 cited

Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries

Nicholas Loutrel, Ava Bailey, Davide Gerosa

Gravitational waves in general relativity are non-dispersive, yet a host of modified theories predict dispersion effects during propagation. In this work, we consider the impact of…

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…

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…

gr-qc2024★ 5 cited

Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit I: General Formalism

Nicholas Loutrel, Sajal Mukherjee, Andrea Maselli +1

We develop a fully analytical waveform model for precessing binaries with arbitrary spin vectors using post-Newtonian~(PN) theory in the extreme mass-ratio limit and a hierarchical…

gr-qc2023★ 6 cited

Relevance of Precession for Tests of the Black Hole No Hair Theorems

Nicholas Loutrel, Richard Brito, Andrea Maselli +1

The multipole moments of black holes in general relativity obey certain consistency relations known as the no-hair theorems. The details of this multipolar structure are imprinted…