Skip to main content
Log in

Third and fourth order resonances in Hamiltonian systems

  • Published:
Celestial mechanics Aims and scope Submit manuscript

Abstract

The stability of the origin of an autonomous Hamiltonian system is investigated when the system possesses a third or fourth-order resonance.H 2, the quadratic part ofH isH 2=∑n i=1 ω i J i and the resonance condition is ∑n i=1 k i ω i where thek ⩾ 0,i = 1, 2, ...,n are the natural or fundamental frequencies. It is shown that the only case in which the origin can be unstable is ifk i≥0,i=1,2,...,n. The condition for instability is then given in terms of the coefficients of the higher order terms in the Hamiltonian. The transfer of energy between modes is also investigated when a near-resonant condition exists.

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

  1. Birkhoff, G. D.: 1966,Am. Math. Soc. Publ. 9, New York.

  2. Cherry, T. M.: 1924, ‘Integrals Developable About a Singular Point of a Hamiltonian System of Differential Equations’, Part II,Proc. Cambridge Philosophical Society 22, 510–533.

    Google Scholar 

  3. Gustavson, F.: 1966,Astron. J. 71, 510.

    Google Scholar 

  4. Arnold, V. I.: 1963,Russian Math. Surveys, London Math. Society.

  5. Markeev, A. P.: 1968,Appl. Math. Mech. 32, 766.

    Google Scholar 

  6. Alfriend, K. T.: 1971,Celest. Mech. 3, 247.

    Google Scholar 

  7. Alfriend, K. T.: 1971,Int. J Nonlinear Mech. 6, 563.

    Google Scholar 

  8. Henrard, J.: 1970,Celest Mech. 1, 437.

    Google Scholar 

  9. Arnold, V. I.: 1968, in L. I. Sedov (ed.),Proceedings of the Second All-Union Conference on Theoretical and Applied Mechanics, 11–14.

  10. Tselman, F. Kh.: 1970,Appl. Math. Mech. 34, 916.

    Google Scholar 

  11. Markeev, A. P.: 1972,Sov. Astron. 682.

  12. Deprit, A.: 1969,Celest. Mech. 1, 12.

    Google Scholar 

  13. Kamel, A. A.: 1969,Celest. Mech. 1, 190.

    Google Scholar 

  14. Garfinkel, B.: 1966,Astron. J. 71, 657.

    Google Scholar 

  15. Breakwell, J. V. and Pringle, R.: 1966, in R. L. Duncombe and V. G. Szebehely, (eds.),Progress in Astronautics and Aeronautics 17, pp. 57–73, Academic Press, N. Y.

    Google Scholar 

  16. Khazin, L. G.: 1971,Appl. Math. Mech. 35, No. 3.

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Alfriend, K.T., Richardson, D.L. Third and fourth order resonances in Hamiltonian systems. Celestial Mechanics 7, 408–420 (1973). https://doi.org/10.1007/BF01227507

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01227507

Keywords

Navigation