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Volumn 60, Issue 5, 1999, Pages 6172-6175

Efficient algorithm for detecting unstable periodic orbits in chaotic systems

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE;

EID: 0001611630     PISSN: 1063651X     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevE.60.6172     Document Type: Article
Times cited : (89)

References (28)
  • 17
    • 0001452580 scopus 로고
    • for the Hénon map for which a Hamiltonian-like function can be found with extrema located at the orbit points of UPO’s;
    • Particular methods exist for specific systems or in special cases, such as the method by Biham and Wenzel [O. Biham and W. Wenzel, Phys. Rev. Lett. 63, 819 (1989)] for the Hénon map for which a Hamiltonian-like function can be found with extrema located at the orbit points of UPO’s
    • (1989) Phys. Rev. Lett. , vol.63 , pp. 819
    • Biham, O.1    Wenzel, W.2
  • 18
    • 26544432046 scopus 로고
    • which is applicable to two-dimensional maps if the symbolic dynamics of the map is known and well ordered
    • and the method by Hansen [K. Hansen, Phys. Rev. E 52, 2388 (1995)] which is applicable to two-dimensional maps if the symbolic dynamics of the map is known and well ordered.
    • (1995) Phys. Rev. E , vol.52 , pp. 2388
    • Hansen, K.1
  • 24
    • 85036375580 scopus 로고    scopus 로고
    • It is practically impossible to use the SD method to detect complete sets of UPO’s for periods above 20 because the amount of computation required grows exponentially at a much higher rate than that of our method
    • It is practically impossible to use the SD method to detect complete sets of UPO’s for periods above 20 because the amount of computation required grows exponentially at a much higher rate than that of our method.
  • 26
    • 85036422410 scopus 로고    scopus 로고
    • Indeed, close to a zero point, the corrections from Eq. (3) are proportional to the deviation (linear convergence), while corrections determined from the NR method yield an error that is proportional to the square of the deviation (quadratic convergence)
    • Indeed, close to a zero point, the corrections from Eq. (3) are proportional to the deviation (linear convergence), while corrections determined from the NR method yield an error that is proportional to the square of the deviation (quadratic convergence).
  • 27
    • 85036170098 scopus 로고    scopus 로고
    • Even though the Newton-Raphson method generally has a fractal basin structure, we show only intervals adjacent to the solution, as they are the most reliable source of starting points
    • Even though the Newton-Raphson method generally has a fractal basin structure, we show only intervals adjacent to the solution, as they are the most reliable source of starting points.
  • 28
    • 85036374785 scopus 로고    scopus 로고
    • For relatively short orbits we verify the completeness of the detected sets by initializing our iteration scheme on a fine grid of initial points
    • For relatively short orbits we verify the completeness of the detected sets by initializing our iteration scheme on a fine grid of initial points.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.