An onset from regular to chaotic regimes through the break-down of a two-dimensional invariant torus has been observed in many natural and man-made systems including the Rayleigh-Benard convection (Jensen et al. 1985), the Taylor-Couette flow (Marques et al. 2001), and electrical circuits (Anishchenko et al. 1993, Baptista and Caldas, 1998).
The detailed numerical experiment on a specific family of maps was performed by Aronson et al. (1982), see also (Curry and Yorke, 1978), . A mathematical description of such a phenomenon in the resonance case was first suggested by Afraimovich and Shilnikov (1983). Previously, Fenichel (1971) showed that the torus always loses its smoothness before the break-down.
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The torus loses its smoothness and eventually disintegrates in three different principal ways. The three scenarios can be described as follows. Assume that for \(0<\varepsilon<\varepsilon_c \) the dynamical system \(f_{\varepsilon}\) has a smooth attracting two-dimensional torus \(T_{\varepsilon} \ ,\) containing an even number of periodic orbits, half of which are stable and half are unstable. The orbits that are unstable on the torus are of saddle-type in the whole phase space of the system. Thus, the torus \(T_{\varepsilon} \) is the closure of the unstable manifolds to the saddle orbits. For the sake of simplicity, assume that there are only two periodic (stable and saddle) orbits on the torus. Let \(\varepsilon_c \) be a bifurcation value. The three scenarios are related to the following bifurcations:
We illustrate these bifurcations by studying a map of an annulus, that models the Poincare map in a neighborhood of a destroyed torus. The specific map is immaterial; for example one may consider the Zaslavsky map in the form \[(x,\theta)\rightarrow (e^{-r}(x+a\sin \theta ),(\theta+r+x+a\sin \theta) \mbox{ mod } 2\pi) \] of the annulus \(0<x \le x_0\ ,\) where \( r >1, a\ge 0, x_0>a/(1-e^{-r})\) (Afraimovich and Hsu 2003).
It is easy to verify that for any integer \(k\) on the plane of parameters \((r,a)\ ,\) the curve\[ B^+: a=\pm(2\pi k-r)(1-e^{-r})\] is a bifurcation curve corresponding to a saddle-node bifurcation of the fixed point. The curve\[ B^-: a^2=(2\pi k-r)^2(1-e^{-r})^2+4(1+e^{-r})^2\] corresponds to the period-doubling bifurcation. There are also bifurcation curves \(B_{1,2}\) corresponding to the tangency of the unstable and stable manifolds of a fixed saddle point from different sides. The bifurcation diagram is shown in Figure 1. For the values of parameters in the pentagonal region bounded by these curves, the map has an invariant curve homeomorphic (but not necessarily diffeomorphic) to the circle.
The paths through \(B^+\) and \(B_{12}\) from the inside are accompanied by the appearance of strange attractors containing infinitely many periodic orbits. The bifurcation on \( B^- \) is the first one in the infinite sequence of period-doubling bifurcations that eventually lead to the appearance of the Feigenbaum attractor and chaotic regimes.
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Internal references
Attractor, Bifurcations, Bubbling Transition, Crises, Dynamical Systems, Periodic Orbit, Stability, Unstable Periodic Orbits