An alternative method to construct a consistent second-order theory on the equilibrium figures of rotating celestial bodies
DOI10.1016/j.cam.2020.113305zbMath1483.70035OpenAlexW3111591125MaRDI QIDQ2059590
Manuel Forner Gumbau, Miguel Barreda-Rochera, José Antonio López Ortí
Publication date: 14 December 2021
Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/j.cam.2020.113305
perturbation theorypotential theoryspherical harmonicscomputational algebrafigures of rotating celestial bodies
Celestial mechanics (70F15) Orbital mechanics (70M20) Stability problems in rigid body dynamics (70E50) Generalized coordinates; event, impulse-energy, configuration, state, or phase space for problems in mechanics (70G10)
Cites Work
- Two algorithms to construct a consistent first order theory of equilibrium figures of close binary systems
- Effects of rotation on internal structure of the stars
- Dynamics of close binary systems
- An improved algorithm of second order to construct consistent theories of equilibrium figures of rotating celestial bodies
- A note on the first-order theories of equilibrium figures of celestial bodies
- The Equilibrium of Distorted Polytropes: (I). The Rotational Problem
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