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Effects of External Noise on Anomalous Diffusion in Hamiltonian Dynamical Systems

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Abstract

The effect of external noise on diffusion processes in a Hamiltonian system with an external force is studied. This is represented by the standard map with an external force. When external noise is applied to the system, we find strongly enhanced diffusion in a parameter range in which anomalous diffusion occurs. Although chaotic orbits are not deterministic in a strict sense, because the system includes noises, they exhibit Lévy flight due to the intermittent sticking to transient tori.

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... For large noise 1/ξ → 0 the exponent evolves as γ → 1 because inner cores become blurred by noise and diffusion is dominant. For intermediate noise intensities some particles intermittently enter within the inner cores where they may remain for some time, while others travel long distances and this causes R 2 (t) to increase superdiffusively [16]. The very high values of γ up to 10 for intermediate noise intensities in Fig. 2(b) can be understood looking at the two curves (red squares and green triangles) in Fig. 2(a). ...
... Above a certain nonzero value of noise intensity the closed flow regimes become permeable to particle crossings which explains the presence of a maximum asymptotic diffusion coefficient. For intermediate noise intensities, D A ∼ ξ −α and the transport becomes superdiffusive [9,10,16]. However, as an important result we find that this dependence does not hold for ξ → 0. The scaling coefficient α was found to decrease with the jet amplitude. ...
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The nontrivial dependence of the asymptotic diffusion on noise intensity has been studied for a Hamiltonian flow mimicking the Gulf Jet Stream. Three different diffusion regimes have been observed depending on the noise intensity. For intermediate noise the asymptotic diffusion decreases with noise intensity at a rate which is linearly dependent to the flow's meander amplitude. Increasing the noise the fluid transport passes through a superdiffusive regime and finally becomes diffusive again at large noise intensities. The presence of inner circulation regimes in the flow has been found to be determinant to explain the observed behavior.
... Since then many different applications and consequences of stickiness were investigated. The onset of anomalous transport is perhaps the most prominent one [Kar83,ISM00,ZT91,ZK94], what will be discussed carefully in Sec. 6.2. ...
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Stickiness refers to chaotic orbits that stay in a particular region for a long time before escaping. For example, stickiness appears near the borders of an island of stability in the phase space of a 2-D dynamical system. This is pronounced when the KAM tori surrounding the island are destroyed and become cantori (see [Contopoulos, 2002]). We find the time scale of stickiness along the unstable asymptotic curves of unstable periodic orbits around an island of stability, that depends on several factors: (a) the largest eigenvalue |λ| of the asymptotic curve. If λ > 0 the orbits on the unstable asymptotic manifold in one direction (fast direction) escape faster than the orbits in the opposite direction (slow direction) (b) the distance from the last KAM curve or from the main cantorus (the cantorus with the smallest gaps) (c) the size of the gaps of the main cantorus and (d) the other cantori, islands and asymptotic curves. The most important factor is the size of the gaps of the main cantorus. Then we find when the various KAM curves are destroyed. The distance of the last KAM curve from the center of an island gives the size of the island. When the central periodic orbit becomes unstable, chaos is also formed around it, limited by a first KAM curve. Between the first and the last KAM curves there are still closed invariant curves. The sizes of the islands as functions of the perturbation, have abrupt changes at resonances. These functions have some universal features but also some differences. A new type of stickiness appears near the unstable asymptotic curves of unstable periodic orbits that extend far into the large chaotic sea. Such a stickiness lasts for long times, increasing the density of points close to the unstable asymptotic curves. However after a much longer time, the density becomes almost equal everywhere outside the islands of stability. We consider also stickiness near the asymptotic curves from new periodic orbits, and stickiness in Anosov systems and near totally unstable orbits. In systems that allow escapes to infinity the stickiness delays the escapes. An important astrophysical application is the case of barred-spiral galaxies. The spiral arms outside corotation consist mainly of sticky chaotic orbits. Stickiness keeps the spiral forms for times longer than a Hubble time, but after a much longer time most of the chaotic orbits escape to infinity.
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IntroductionContinuous Time RandomWalk ModelOrigin of Long-Time Tails in Hamiltonian SystemParadigmatic Fluid ModelDiscussionReferences
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