Milankovitch equations with spinors
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Publication:6076465
DOI10.1007/s10569-023-10162-3arXiv2212.05929OpenAlexW4387120106MaRDI QIDQ6076465
Jean-Baptiste Fouvry, Barnabás Deme
Publication date: 17 October 2023
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2212.05929
Poisson bracketsecular dynamicsoblate planetKozai-Lidov mechanismcanonical variablequasi-Keplerian system
Cites Work
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- On the Milankovitch orbital elements for perturbed Keplerian motion
- Quaternions and the perturbed Kepler problem
- New foundations for classical mechanics
- The solution of the \(n\)-body problem
- Integrability and chaos: the classical uncertainty
- Celestial mechanics with geometric algebra
- The Three-Body Problem
- The Gravitational Million–Body Problem
- Solar System Dynamics
- Collective symplectic integrators
- Perturbation theory of Kepler motion based on spinor regularization.
- Runge–Lenz vector as a 3d projection of SO(4) moment map in R4×R4 phase space
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