Séminaire / Seminar GReCO |
« Solution to binary black hole dynamics » |
Sashwat Tanay |
Accurate and efficient modeling of binary black holes (BBHs) is crucial for the detection of gravitational waves (GWs) emitted by them. Closed-form solutions to these systems are highly sought after and have been worked out by many groups in the past few decades. Most of these solutions are valid only in certain limits (small eccentricity, zero spins, equal mass binary, etc). In this talk, we will discuss our recently derived solution for the most general BBH system (with arbitrary masses, eccentricity, and spins). Two newly discovered constants of motion will also be presented. |
lundi 29 janvier 2024 - 11:00 Salle des séminaires Évry Schatzman Institut d'Astrophysique de Paris |
Pages web du séminaire / Seminar's webpage |