We consider dissipative one-dimensional systems subject to a periodic force. As a model system, particularly suited for numerical analysis, we investigate the driven cubic oscillator in the presence of friction, and study numerically how time-varying friction affects the dynamics. We find that, if the damping coefficient increases in time up to a final constant value, then the basins of attraction of the leading resonances are larger than they would have been if the coefficient had been fixed at that value since the beginning. From a quantitative point of view, the scenario depends both on the final value and the growth rate of the damping coefficient. The relevance of the results for the spin-orbit model is argued and discussed in some detail.

Bartuccelli, M., Deane, J., Gentile, G. (2012). Attractiveness of periodic orbits in parametrically forced systems with time-increasing friction. JOURNAL OF MATHEMATICAL PHYSICS, 53(10), 102703-1-102703-27 [10.1063/1.4757650].

Attractiveness of periodic orbits in parametrically forced systems with time-increasing friction

GENTILE, Guido
2012-01-01

Abstract

We consider dissipative one-dimensional systems subject to a periodic force. As a model system, particularly suited for numerical analysis, we investigate the driven cubic oscillator in the presence of friction, and study numerically how time-varying friction affects the dynamics. We find that, if the damping coefficient increases in time up to a final constant value, then the basins of attraction of the leading resonances are larger than they would have been if the coefficient had been fixed at that value since the beginning. From a quantitative point of view, the scenario depends both on the final value and the growth rate of the damping coefficient. The relevance of the results for the spin-orbit model is argued and discussed in some detail.
2012
Bartuccelli, M., Deane, J., Gentile, G. (2012). Attractiveness of periodic orbits in parametrically forced systems with time-increasing friction. JOURNAL OF MATHEMATICAL PHYSICS, 53(10), 102703-1-102703-27 [10.1063/1.4757650].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/122081
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