Library

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Celestial mechanics and dynamical astronomy 5 (1972), S. 407-427 
    ISSN: 1572-9478
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract In many cases, the evolution of a Hamiltonian system can be represented by an area-preserving mapping of the plane onto itself. The stability or instability of the dynamical system is reflected in the derived mapping. The mappingT(x, y)=(x', y'): $$\begin{gathered} x\prime = x + a(y - y^3 ) \hfill \\ y\prime = y - a(x\prime - x\prime ^3 ) \hfill \\ \end{gathered} $$ was studied in order to determine methods of readily compartmentalizing the plane into regions of stable and unstable behavior under many applications ofT, without resorting to costly and frequently inaccurate methods requiring computation of thousands of maps. The concept of separatrices, which exist for perfectly integrable systems, is replaced by the more general idea of extended eigenvectors from hyperbolic fixed points of the mappings, where the eigenvectors are those of the matrix representing the mapping linearized in the neighborhood of the fixed point. It was demonstrated by Bartlett that these extended eigenvectors, or eigencurves, from neighboring hyperbolic fixed points, may intersect each other to form intricate networks of intersecting loops. This area will be stable if the ratio of loop area to cell area is very small, of the order of 10−5 for the above mapping. Generally, if the oscillation cannot be seen, one should act as if the entire area of the cell is stable.
    Type of Medium: Electronic Resource
    Library Location Call Number Volume/Issue/Year Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...