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Damped, Oscillatorily Driven Pendulum Motion

A ball of mass m is attached to a stiff, but massless rod of length l . Gravity acts on it, providing a force m g sin ( θ ) perpendicular to the rod. The pendulum is also damped by a force γ ω and driven by an oscillatory force F 0 cos ( ω d t ) . Thus, the equations of motion are m l α = m g sin ( θ ) γ ω + F 0 cos ( ω d t ) . The constants used are l = g = m = 1 , γ = 0.05 , F 0 = 0.7 , and ω d = 0.7 . Poincare plots and phase plots of this system are respectively shown below.

image Poincare plots of three initial conditions. Blue: θ = 0 , ω = 1 . Red: θ = 0.6 , ω = 0.8 . Purple: θ = 1 , ω = 0 . (above)

image Modded phase plot of initial condition θ = 1 , ω = 0 ; ϕ is time t modulo 2 π / ω d . (above)

image Phase plots over time for the three initial conditions. Blue: θ = 0 , ω = 1 . Red: θ = 0.6 , ω = 0.8 . Purple: θ = 1 , ω = 0 . (above)

image Phase plots over time for the three initial conditions. Blue: θ = 0 , ω = 0.9999 . Red: θ = 0 , ω = 1.0001 . Purple: θ = 0 , ω = 1 . (above)

As seen, close initial conditions can diverge after a short amount of time. However, as the paths do not interesect, the motion is deterministic.

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A demonstration of chaos in a driven pendulum.

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