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Explore the eccentric dynamics of black hole binary systems in this 14-minute talk by Akash Maurya from the International Centre for Theoretical Sciences. Presented during the 2nd Session of the In House 2025 Symposium on April 22, 2025, the presentation introduces ESIGMAHM as a tool for investigating the non-circular orbital behaviors of binary black hole systems. Learn about the latest theoretical approaches to understanding these complex astrophysical phenomena and their implications for gravitational wave astronomy.
