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Introducing SINFONIA: Symplectic, slimplectic and Magnusian (Neural) Flows for Orbital Numerical Integration and Acceleration

Da Silva, Lidia J. Gomes
arXiv (All) · Papers
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computational-physicsgeneral-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenamachine-learning
Long-duration gravitational-wave modelling must resolve fast orbital motion together with slow dissipative evolution while preventing small numerical errors from accumulating into secular phase drift. Here we ask whether the finite-time evolution map itself can be learned as an explicit, differentia
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