English

Numerical integration of variational equations

Chaotic Dynamics 2015-03-17 v3 Earth and Planetary Astrophysics Astrophysics of Galaxies Mathematical Physics math.MP Computational Physics

Abstract

We present and compare different numerical schemes for the integration of the variational equations of autonomous Hamiltonian systems whose kinetic energy is quadratic in the generalized momenta and whose potential is a function of the generalized positions. We apply these techniques to Hamiltonian systems of various degrees of freedom, and investigate their efficiency in accurately reproducing well-known properties of chaos indicators like the Lyapunov Characteristic Exponents (LCEs) and the Generalized Alignment Indices (GALIs). We find that the best numerical performance is exhibited by the \textit{`tangent map (TM) method'}, a scheme based on symplectic integration techniques which proves to be optimal in speed and accuracy. According to this method, a symplectic integrator is used to approximate the solution of the Hamilton's equations of motion by the repeated action of a symplectic map SS, while the corresponding tangent map TSTS, is used for the integration of the variational equations. A simple and systematic technique to construct TSTS is also presented.

Keywords

Cite

@article{arxiv.1006.0154,
  title  = {Numerical integration of variational equations},
  author = {Ch. Skokos and E. Gerlach},
  journal= {arXiv preprint arXiv:1006.0154},
  year   = {2015}
}

Comments

27 pages, 11 figures, to appear in Phys. Rev. E

R2 v1 2026-06-21T15:30:30.912Z