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Learn about the self-force (SF) approximation scheme in gravitational physics through this 32-minute conference talk delivered at the QCD meets Gravity XI Conference. Explore the theoretical framework and mathematical foundations of the SF approximation method, which plays a crucial role in understanding gravitational wave physics and binary black hole systems. Gain insights into how this computational approach helps bridge the gap between analytical and numerical relativity, particularly in modeling extreme mass ratio inspirals and other gravitational phenomena. Discover the applications and limitations of the SF scheme in contemporary gravitational wave research and its significance for LIGO/Virgo detections and future space-based gravitational wave missions.
