GJC: Matteo Boschini "Eccentricity: a recipe from catastrophe"

Europe/Rome
Sala Lauree (Marconi)

Sala Lauree

Marconi

Description
While the orbital eccentricity is a key feature of the gravitational two-body problem, providing an unambiguous definition in General Relativity poses significant challenges. Despite such foundational issues, the eccentricity of binary black holes has important implications in gravitational-wave astronomy. This work presents a novel approach to consistently define the orbital eccentricity in General Relativity, grounded in the mathematical field of catastrophe theory. Specifically, we identify the presence of catastrophes —i.e. breakdowns of the stationary-phase approximation— in numerical-relativity waveforms and exploit them to develop a robust and fully gauge-invariant estimator of the eccentricity. Our procedure does not require orbital fitting and naturally satisfies the Newtonian limit. We extract gauge-free eccentricity estimates from about 100 numerical-relativity simulations and find that the resulting values are systematically lower compared to those reported alongside the simulations themselves.
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