A Symplectic Trigonometrically Fitted Modified Partitioned Runge-Kutta Method for the Numerical Integration of Orbital Problems
DOI10.1002/ANAC.200510037zbMath1084.65128OpenAlexW1996028789MaRDI QIDQ5717700
Th. Monovasilis, Zacharoula Kalogiratou, Theodore E. Simos
Publication date: 10 January 2006
Published in: Applied Numerical Analysis & Computational Mathematics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1002/anac.200510037
two-body problemHamiltonian systemsharmonic oscillatortrigonometrically fitted methodsSymplectic integration
Two-body problems (70F05) Multistep, Runge-Kutta and extrapolation methods for ordinary differential equations (65L06) Orbital mechanics (70M20) Numerical methods for Hamiltonian systems including symplectic integrators (65P10) Discretization methods and integrators (symplectic, variational, geometric, etc.) for dynamical systems (37M15) Free motions in linear vibration theory (70J30)
Related Items (3)
Cites Work
- An exponentially-fitted Runge-Kutta method for the numerical integration of initial-value problems with periodic or oscillating solutions
- Exponentially-fitted explicit Runge-Kutta methods
- Stabilization of Cowell's method
- Extended One-Step Methods: An Exponential Fitting Approach
- The accuracy of symplectic integrators
- Exponentially-fitted algorithms: fixed or frequency dependent knot points?
- Effective Numerical Approximation of Schrödinger type Equations through Multiderivative Exponentially-fitted Schemes
- Efficient Numerical Solution of Orbital Problems with the use of Symmetric Four-step Trigonometrically-fitted Methods
- Non-existence of the modified first integral by symplectic integration methods
This page was built for publication: A Symplectic Trigonometrically Fitted Modified Partitioned Runge-Kutta Method for the Numerical Integration of Orbital Problems