CORDIS Project
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The MoGEs project focuses on modeling the dynamics of compact binary systems to improve the understanding of gravitational waves. It aims to incorporate various factors such as spin and eccentricity to enhance predictions for future gravitational wave observatories.
Inspiralling binaries of compact objects are a promising source of gravitational waves (GWs) in the upcoming era of GW astronomy.
The MoGEs project proposes to take the next step in modelling the evolution of compact binaries using the gravitational self-force (GSF) formalism.
Until now, the linear-in-mass-ratio GSF has only been calculated under the simplifying assumptions of non-spinning, circular, and/or equatorial binaries.
MoGEs will, for the first time, calculate linear-in-mass-ratio GSF i…
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
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