2013
DOI: 10.1016/j.aop.2012.11.018
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Newton–Hooke-type symmetry of anisotropic oscillators

Abstract: The rotation-less Newton-Hooke -type symmetry found recently in the Hill problem and instrumental for explaining the center-of-mass decomposition is generalized to an arbitrary anisotropic oscillator in the plane. Conversely, the latter system is shown, by the orbit method, to be the most general one with such a symmetry. Full Newton-Hooke symmetry is recovered in the isotropic case.Star escape from a Galaxy is studied as application.

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Cited by 25 publications
(24 citation statements)
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“…(2.14) is well known, in our case it is a linear combinations of trigonometric functions only or both hyperbolic (or linear) and trigonometric ones depending on the values of parameters appearing in (2.14), the form of the coefficients can be quite complicated (for γ = they are presented in [21]). In the general case the transformation to the normal coordinates seems more useful (see also [54,55]). The above results form a setup for our further considerations.…”
Section: )mentioning
confidence: 99%
“…(2.14) is well known, in our case it is a linear combinations of trigonometric functions only or both hyperbolic (or linear) and trigonometric ones depending on the values of parameters appearing in (2.14), the form of the coefficients can be quite complicated (for γ = they are presented in [21]). In the general case the transformation to the normal coordinates seems more useful (see also [54,55]). The above results form a setup for our further considerations.…”
Section: )mentioning
confidence: 99%
“…According to the Robertson Theorem ( [7] (Sec. 8.1.3., p. 169), see also [8]), classical separability does imply, in our case, that of the Schrödinger equation 4. Restricting ourselves to natural orthogonal systems, i.e., such whose Hamiltonian is H = 1 2 n k=1 g k (x 1 , .…”
Section: Classical Separabilitymentioning
confidence: 99%
“…(2.15). Our theory provides us now with D = 2 conserved quantities in involution, namely with the separable 2D Hamiltonian, 4) and with the Runge-Lenz-type conserved quantity…”
Section: Reduction To and Induction From The 2d Problemmentioning
confidence: 99%
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