Self-Consistent Spin, Tidal, and Dynamical Equations of Motion in REBOUND Framework

Learn about the integration of equilibrium tide theory into the REBOUND N-body simulator in this 52-minute physics lecture from Yale researcher Tiger Lu. Explore how accounting for structural effects beyond point particle approximation enhances planetary dynamics simulations. Gain insights into the self-consistent modeling of tidal interactions, rotational deformation, and planetary rotation through the EKH framework. Follow the implementation details and performance benchmarking against analytic predictions, including applications to hot Jupiter spin dynamics and spin-orbit resonances. Examine comparisons with secular expressions and ML19 results while discovering future research directions in this comprehensive overview of advanced planetary dynamics simulation techniques.