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multiple time scale dynamics with two fast variables and one slow ...

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has a homoclinic orbit x0(t). We are interested in perturbations <strong>with</strong> s>0 <strong>and</strong><br />

note that in this case the divergence of (3.10) is s. Hence the vector field is<br />

area exp<strong>and</strong>ing everywhere. The homoclinic orbit breaks for s > 0 <strong>and</strong> no<br />

periodic orbits are created. Note that this scenario does not apply to the full<br />

three-dimensional system as the equilibrium q has a pair of complex conjugate<br />

eigenvalues so that a Shil’nikov scenario can occur. This illustrates that the sin-<br />

gular limit can be used to help locate homoclinic orbits of the full system, but<br />

that some characteristics of these orbits change in the singular limit.<br />

We are interested next in finding curves in ( ¯p, s)-parameter space that rep-<br />

resent heteroclinic connections of the <strong>fast</strong> subsystem. The main motivation is<br />

the decomposition of trajectories in the full system into <strong>slow</strong> <strong>and</strong> <strong>fast</strong> segments.<br />

Concatenating <strong>fast</strong> heteroclinic segments <strong>and</strong> <strong>slow</strong> flow segments can yield ho-<br />

moclinic orbits of the full system [62, 15, 69, 82]. We describe a numerical strat-<br />

egy to detect heteroclinic connections in the <strong>fast</strong> subsystem <strong>and</strong> continue them<br />

in parameter space. Suppose that ¯p∈( ¯pl, ¯pr) so that (3.10) has three hyperbolic<br />

equilibrium points xl, xm <strong>and</strong> xr. We denote by W u (xl) the unstable <strong>and</strong> by W s (xl)<br />

the stable manifold of xl. The same notation is also used for xr <strong>and</strong> tangent<br />

spaces to W s (.) <strong>and</strong> W u (.) are denoted by T s (.) <strong>and</strong> T u (.). Recall that xm is a source<br />

<strong>and</strong> shall not be of interest to us for now. Define the cross sectionΣby<br />

Σ={(x1, x2)∈R 2 : x1= xl+xr<br />

}.<br />

2<br />

We use forward integration of initial conditions in T u (xl) <strong>and</strong> backward integra-<br />

tion of initial conditions in T s (xr) to obtain trajectoriesγ + <strong>and</strong>γ − respectively.<br />

We calculate their intersection <strong>with</strong>Σ<strong>and</strong> define<br />

γl( ¯p, s) :=γ + ∩Σ, γr( ¯p, s) :=γ − ∩Σ<br />

71

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