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Chirikov Standard Map - KAM Tori

What you are seeing: the simplest area-preserving map that exhibits the transition from regular motion to chaos. At each step we kick a rotator and let it free-rotate; the result is a discrete Hamiltonian dynamics on the torus (θ,p)[0,2π)2(\theta, p) \in [0, 2\pi)^2. The rule is pn+1=pn+Ksin(θn)p_{n+1} = p_n + K\sin(\theta_n), θn+1=θn+pn+1\theta_{n+1} = \theta_n + p_{n+1} (both mod 2π2\pi).

At K=0K = 0 the dynamics is integrable: every horizontal line p=constp = \text{const} is invariant, and trajectories fill it densely if p/2πp/2\pi is irrational or close to it in a Diophantine sense. As KK grows, the KAM theorem guarantees that "sufficiently irrational" tori survive while rational tori shatter into chains of islands and surrounding chaos. The most persistent torus has the golden-mean winding number (51)/2(\sqrt 5 - 1)/2 and breaks last, at the critical value Kcrit0.9716K_\text{crit} \approx 0.9716. Above this value, orbits can in principle diffuse arbitrarily far in pp.

Click anywhere on the plot to seed a new orbit at that (θ,p)(\theta, p). Each color is a separate initial condition. Drag the KK slider and watch the regular curves break up.

Figure 1. Phase portrait of the Chirikov standard map. Method: 32 initial conditions, 1200 forward iterates each.
K0.971
n/orbit1200

WHAT TO TRY

  • Raise the kick strength K from zero: at K = 0 the rotor sits on clean horizontal lines (conserved tori), and as K grows islands and a chaotic sea appear between them. The phase space goes mixed.
  • Push K past the critical 0.9716: the last KAM torus spanning the map breaks, and trajectories can finally wander across the whole momentum range. That threshold is where global chaos sets in.
  • Seed the rotor inside an island versus in the chaotic sea: island orbits stay regular and bounded, sea orbits fill space erratically, both living in the same phase portrait.