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04 Chaotic Pendulum

Aim

To analyze the chaotic motion of a parametrically driven pendulum by explaining its motion in phase space by making a Poincaré plot.

Subjects

Diagram

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Figure 1:.

Equipment

Presentation

The Pendulum is fixed on the shaft of the rotary motion sensor. The rotary motion sensor is fixed to the slide that is driven up and down by a crank mechanism (See Diagram and Figure 3 1).

The driven pendulum, see Figure 2, is placed on a spot that can be observed by all the students but which can be closed off during the lecture i self. Place it for example just outside the lecture room, so the door can be shut during the lecture, while keeping the monitor image visible to the students

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Figure 2:.

The software is set up to make a Poincaré plot of the angular position and angular velocity, and will be projected in the lecture room with use of the projector. The Poincaré plot will grow during the lecture and after a while the strange chaotic attractor will be displayed. In about 1 hour you will be able to see the contours of the attractor; after an other hour you will have a plot like in Figure 3.

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Figure 3:.

At the beginning of the lecture, having started the driven pendulum, you can introduce the driven pendulum and show its chaotic behavior. After this you can explain why we use a Poincaré plot to analyze the chaotic movement of the pendulum and that in a Poincaré plot not the time but space determines when to plot a point, by showing the students the spot where both angular position and angular frequency is measured en plotted against each other in the Poincaré plot.

Explanation

The equation of motion of a Chaotic pendulum is (see: SourcesXX):

d2ϑdt2+k2mL2dϑdt+[ω2AΩ2Lcos(Ωt)]sin(ϑ)=0\frac{d^{2} \vartheta}{d t^{2}}+\frac{k_{2}}{m L^{2}} \frac{d \vartheta}{d t}+\left[\omega^{2}-\frac{A \Omega^{2}}{L} \cos (\Omega t)\right] \sin (\vartheta)=0

where:

If there is no damping, k2=0k_{2}=0. If there is no driving force, A=0A=0. Then the equation of motion will be:

d2ϑdt2+ω2sin(ϑ)=0\frac{d^{2} \vartheta}{d t^{2}}+\omega^{2} \sin (\vartheta)=0

When we substitute, ω=gL\omega=\sqrt{\frac{g}{L}} and L=ImL=\frac{I}{m \ell}, we will get the following equation of motion:

d2ϑdt2+mgIsin(ϑ)=0\frac{d^{2} \vartheta}{d t^{2}}+\frac{m g \ell}{I} \sin (\vartheta)=0

Solving this differential equation yields:

12ϑ2mgIcos(ϑ)= const. (McComb equation 6.25). \frac{1}{2} \vartheta^{2}-\frac{m g \ell}{I} \cos (\vartheta)=\text { const. (McComb equation 6.25). }

The Parametrically driven pendulum is based on the article, *Unstable periodic orbits in the parametrically excited pendulum, of W. van der Water.*In this article some more friction terms have been added to the equation of motion of the chaotic pendulum, so that result of the simulation and the actual experiment are more like each other.

Remarks

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Figure 4:.

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Figure 5:.

Sources