Skip to main content
Log in

Numerical treatment of non-integrable dynamical systems

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

A systematic and detailed discussion of the ‘gravitational’ spring-pendulum problem is given for the first time. A procedure is developed for the numerical treatment of non-integrable dynamical systems which possess certain properties in common with the gravitational problem. The technique is important because, in contrast to previous studies, it discloses completely the structure of two-dimensional periodic motion by examining the stability of the one-dimensional periodic motion. Through the parameters of this stability, points have been predicted from which the one-dimensional motion bifurcates into two-dimensional motion. Consequently, families of two-dimensional periodic solutions emanated from these points are studied. These families constitute the generators of the mesh of all the families of periodic solutions of the problem.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Kazantzis, P.G. Numerical treatment of non-integrable dynamical systems. Astrophys Space Sci 61, 287–316 (1979). https://doi.org/10.1007/BF00640533

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00640533

Keywords

Navigation