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Collaborator: D.V. Turaev
Cooperation with: S.V. Gonchenko, L.P. Shilnikov (Institute for Applied Mathematics and Cybernetics, Nizhny Novgorod, Russia)
Supported by: DFG grant no. 436 RUS, Prize of the Alexander von Humboldt Foundation
Description:
Since Poincaré's pioneering work, orbits which are homoclinic to saddle periodic ones have been one of the most attractive objects of study in the theory of dynamical systems. The main reason to study homoclinic orbits is that their presence implies complicated dynamics. It is well known that in any neighborhood of a transverse homoclinic orbit there exist infinitely many saddle periodic orbits and a continuum of nontrivial hyperbolic recurrent orbits. If the system has a nontransverse homoclinic orbit, that is, in the case of homoclinic tangency, then in any neighborhood of the given system there exist infinitely many Newhouse regions where systems with homoclinic tangencies are dense.
Since Newhouse regions exist near any system with a homoclinic tangency, it follows that they can be found in the space of parameters of any dynamical model demonstrating chaotic behavior in absence of uniform hyperbolicity, in particular in such popular examples as Hénon map, Chua circuit, Lorenz model, etc. Moreover, as numerics shows, the Newhouse regions can occupy quite large portions of the parameter space. Therefore, the problem of understanding the nature of the orbit structure for systems from Newhouse regions is quite challenging.
We have found that the dynamics of systems from the Newhouse regions is extremely rich and unusual (see Project 2). As it was shown in [2], a description of the dynamics of such systems requires an infinite set of invariants which means that any attempt to give a complete description of the dynamics and bifurcations in the Newhouse regions will fail. Therefore, we have to restrict the analysis to some particular details or to some most general features only.
As the most important of such general properties of systems in the Newhouse regions, we select the coexistence of many periodic orbits of different stability types (i.e., with different numbers of positive/negative Lyapunov exponents). It has been demonstrated in [1] that stable periodic orbits can coexist with saddle ones near a homoclinic tangency in threedimensional systems. The questions which conditions provide the same phenomenon in the multidimensional case and which conditions could lead to the coexistence of saddles of different types within the regions of chaotic dynamics were raised by many authors. In the present work [4] we give a complete answer to these questions for systems from the Newhouse regions.
Consequently, following [3], we classify codimension1 homoclinic tangencies by the value of the socalled effective dimension d_{e}. It is an integer which can be effectively computed for any given system with a homoclinic tangency. We have proven the following result.
Theorem 1. In the Newhouse regions the values of parameters are dense (and form a residual set) for which the system has infinitely many coexisting hyperbolic periodic orbits of (d_{e}+1) different stability types.
We describe exactly the types of these periodic orbits for different types of the Newhouse regions and show that orbits of other stability types cannot exist here. So, the question for the maximal and minimal number of positive Lyapunov exponents of the orbits of systems under consideration, as well as the question for the coexistence of orbits with different numbers of positive Lyapunov exponents, has been solved completely. In particular, we obtain necessary and sufficient conditions for the denseness of systems with infinitely many stable periodic orbits in the Newhouse regions.
We also address the question for the coexistence of infinitely many nontrivial attractors. We have proven the following result.
Theorem 2. In the case , the values of parameters in the Newhouse regions are dense and form a residual set for which the system has infinitely many coexisting stable invariant tori.
The problem of the coexistence of infinitely many strange attractors in the case was also discussed in [4].
Description:
It has been proved in [2] that systems with homoclinic tangencies of arbitrarily high order are dense in the Newhouse regions, as well as systems having degenerate periodic orbits with all Lyapunov coefficients equal to zero. This implies that bifurcations of such systems are extremely involved and rich. Thus, the question arises: Can we estimate in exact terms how rich these bifurcations are? In [5] we give a definite answer for the example of twodimensional areapreserving maps. It is shown that we deal here with the ultimate richness: Every possible dynamics can be obtained by a small perturbation of any system from a Newhouse region.
To be more precise, let f be a C^{r}smooth areapreserving map of R^{2}. Define the dynamical conjugacy class of f as the set of all maps of a unit disc U_{1} into R^{2} obtained by the rule , where n is an integer, f^{n} is the nth iteration of f, and is an arbitrary C^{r}smooth map of U_{1} into R^{2} with a constant Jacobian (hence, by construction, all the maps in the class are area preserving).
When we speak about the dynamics of a map, then we somehow describe its iterations, where the description should be independent of smooth coordinate transformations. Therefore, the class of maps f just introduced yields some representation of the dynamics of f. Note that the coordinate transformations are not area preserving (they preserve the standard symplectic form up to a constant factor), i.e., the image can be a disc of an arbitrarily small radius with its center located anywhere. Thus, the class of maps f contains information about the behavior of arbitrarily long iterations of f on arbitrarily fine spatial scales.
The general intuition here is that if the class of maps is large, then the dynamics is rich, while if the dynamics is sufficiently simple, then the class is somehow restricted. The following definition introduces maps whose dynamics is ultimately rich.
Definition. A C^{r}smooth symplectic map f is called universal (or C^{r}universal) if its dynamical class is dense in the C^{r}topology among all C^{r}smooth symplectic diffeomorphisms .
By this definition, the detailed understanding of the dynamics of any single universal map is not simpler than the understanding of all other areapreserving maps altogether, i.e., it is beyond human abilities. What is astonishing, is that such universal maps are quite common. Namely, we show in [5] that the following statement is valid.
Theorem 3. C^{r}universal maps exist in any neighborhood
(in the C^{r}topology) of any areapreserving map with a homoclinic
tangency, i.e., they are dense in the Newhouse regions.
This theorem says that universal maps occur as often as homoclinic
tangencies do. It is an empirical fact that if we have any explicitly
given areapreserving map with chaotic behavior, then by slightly
changing parameters
we can quite often encounter a homoclinic tangency.
Thus, according to the theorem above, if we have enough control
parameters then
we can tune our map as close as we want to any
other areapreserving map in some carefully chosen coordinates.
Cooperation with: L.P. Shilnikov (Institute for Applied Mathematics and Cybernetics, Nizhny Novgorod, Russia)
Supported by: Prize of the Alexander von Humboldt Foundation
Description: The problem of synchronization is one of the main problems of applied signal processing. It can be formulated as follows: Let a generator of periodic oscillations be forced by an external periodic signal. Under which conditions will the generator respond with the same frequency as the external signal? Can it respond to the signal with a fractional or multiple frequency? Which response should we expect in general?
When the amplitude of the external force is small, these questions are solved by the classical method of averaging: depending on the frequency detuning, either synchronization or beating regimes should be expected. In the case of finite amplitude, the situation becomes much more complicated: synchronization of different frequencies is possible for the same parameter values, as well as chaotic regimes. In [6] we study the problem of sudden transition from synchronization to chaos. This process can be modeled in geometrical terms as a bifurcation of a saddlenode periodic orbit with a nonsmooth homoclinic loop (see Figure 1). We give criteria which allow to distinguish between two possible scenarios of what happens when the saddlenode has disappeared: either the dynamics is always chaotic, or zones of chaotic behavior interchange in the parameter space with zones of synchronization.
We also analyze in [6] the problem of coexistence of chaotic and synchronized behavior. The classical result of Cartwright and Littlewood from 1945 [7] (explaining earlier experiments by van der Pol) is that the coexistence of two synchronization regimes with different frequencies implies also the existence of a chaotic transient. We enhanced this by giving criteria for the coexistence of chaos with a single synchronized regime and for the existence of chaos in the absence of stable synchronized regimes.

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