THE CREATION OF HORSESHOES

被引:53
作者
HALL, T
机构
[1] Dept. of Appl. Math. and Theor. Phys., Cambridge Univ.
关键词
D O I
10.1088/0951-7715/7/3/008
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
We present results which describe constraints on the order in which periodic orbits can appear when a horseshoe is created. We associate two rational numbers q(R) and r(R) to each periodic orbit R of the horseshoe, which have the property that if r(R) < q(S) then the orbit R must appear after the orbit S; while if r (S) < r (R) and q (R) < q (S) then either orbit can appear before the other. The time required to compute these quantities is bounded by a linear function of the period of R. We also present an algorithm for determining the rotation interval of a horseshoe orbit, and describe techniques for obtaining lower bounds on the topological entropy of a horseshoe orbit.
引用
收藏
页码:861 / 924
页数:64
相关论文
共 50 条
[41]  
Rolfsen D, 1976, KNOTS LINKS, V7
[42]   THE GEOMETRY OF MARKOV NUMBERS [J].
SERIES, C .
MATHEMATICAL INTELLIGENCER, 1985, 7 (03) :20-29
[43]  
Sharkovskii A.N., 1964, INT J BIFURCAT CHAOS, V16, P61
[44]   RELATIVE ROTATION RATES FOR DRIVEN DYNAMICAL-SYSTEMS [J].
SOLARI, HG ;
GILMORE, R .
PHYSICAL REVIEW A, 1988, 37 (08) :3096-3109
[45]   ON THE GEOMETRY AND DYNAMICS OF DIFFEOMORPHISMS OF SURFACES [J].
THURSTON, WP .
BULLETIN OF THE AMERICAN MATHEMATICAL SOCIETY, 1988, 19 (02) :417-431
[46]  
TRESSER C, 1978, CR ACAD SCI A MATH, V287, P577
[47]  
VAN STRIEN S. J., 1981, LECT NOTES MATH, V898, P316
[48]  
Wiggins S., 1988, GLOBAL BIFURCATIONS
[49]  
Wright E., 1979, INTRO THEORY NUMBERS
[50]  
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