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0002199501
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V. G. Gurzadyan, D. Pfenniger, Springer, Berlin
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H. Wozniak, in Ergodic Concepts in Stellar Dynamics, edited by V. G. Gurzadyan and D. Pfenniger (Springer, Berlin, 1994), p. 264
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Wozniak, H.1
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See, e.g., S. Bleher, C. Grebogi, and E. Ott, Physica D 46, 87 (1990)
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Bleher, S.1
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4243069828
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and references cited therein
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Y.-T. Lau, J. M. Finn, and E. Ott, Phys. Rev. Lett. 66, 978 (1991), and references cited therein.
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29
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85036281571
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(private communication)., In any event, determining with great precision the exact boundary of the sticky region for unperturbed orbits is not well motivated physically: Once the orbit has been perturbed, the value of its energy will have changed, which implies that the boundary is no longer the same
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G. Contopoulos (private communication);J. D. Meiss (private communication).In any event, determining with great precision the exact boundary of the sticky region for unperturbed orbits is not well motivated physically: Once the orbit has been perturbed, the value of its energy will have changed, which implies that the boundary is no longer the same.
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Contopoulos, G.1
Meiss, J.D.2
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31
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0001286323
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M. E. Mahon, R. A. Abernathy, B. O. Bradley, and H. E. Kandrup, Mon. Not. R. Astr. Soc. 275, 443(1995).
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Kandrup, H.E.4
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38
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85036333975
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This anomalous behavior tends to arise most often for very small values of (Formula presented) which suggests that, for sufficiently low amplitude, noise is not all that helpful in allowing an ensemble which has already dispersed to find holes in the confining cantori
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This anomalous behavior tends to arise most often for very small values of (Formula presented) which suggests that, for sufficiently low amplitude, noise is not all that helpful in allowing an ensemble which has already dispersed to find holes in the confining cantori.
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39
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4243573090
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See, in particular, Fig. 33
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A. J. Lichtenberg and B. P. Wood, Phys. Rev. Lett. 62, 2213 (1989). See, in particular, Fig. 33.
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Lichtenberg, A.J.1
Wood, B.P.2
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