Coupled Oscillator: Double Pendulum

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By Jimmy Apablaza

This problem is described in Page 321-322, Section 7.6 of the A first Course in Differential Equations textbook, 8ED (ISBN 0-534-41878-3).

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Figure 1. Coupled Pendulum.‎

Problem Statement

Consider the double-pendulum system consisting of a pendulum attached to another pendulum shown in Figure 1.

Assumptions:

  • the system oscillates vertically under the influence of gravity.
  • the mass of both rod are negligible
  • no damping forces act on the system
  • positive direction to the right.

The system of differential equations describing the motion is nonlinear

(m1+m2)l12θ1+m2l1l2θ2cos(θ1θ2)+m2l1l2(θ2)2sin(θ1θ2)+(m1+m2)l1gsinθ1=0
m2l12θ2+m2l1l2θ1cos(θ1θ2)m2l1l2(θ1)2sin(θ1θ2)+m2l2gsinθ2=0


In order to linearize these equations, we assume that the displacements θ1 and θ2 are small enough so that cos(θ1θ2)1 and sin(θ1θ2)0. Thus,

(m1+m2)l12θ1+m2l1l2θ2+(m1+m2)l1gθ1=0
m2l12θ2+m2l1l2θ1+m2l2gθ2=0

Solution

Since our concern is about the motion functions, we will assign the masses m1 and m2, the rod lenghts l1 and l1, and gravitational force g constants to different variables as follows,

A=(m1+m2)l12B=m2l1l2C=(m1+m2)l1gD=m2l12E=m2l2g

Hence,

Aθ1'+Bθ2'+Cθ1=0
Dθ2'+Bθ1'+Eθ2=0

Solving for θ1' and θ2' we obtain,

θ1'=(BA)θ2'(CA)θ1
θ2'=(BD)θ1'(ED)θ2

Therefore,

θ1'=(CDAD+B2)θ1(BEAD+B2)θ2
θ2'=(BCAD+B2)θ1(AEAD+B2)θ2

State Space

[θ1'θ1'θ2'θ2']=A^x_(t)+B^u_(t)=[0100CDADB20BEADB200001BCADB20AEADB20]{θ1θ1'θ2θ2'}+0^

Let's plug some numbers. It's known that g=32. In addition, we assume that m1=3, m2=1, and l1=l2=16, so the constants defined previously become,

A=1024B=256C=2048D=256E=512

Hence, the state space matrix is,

[θ1'θ1'θ2'θ2']=[01008302300001830830]{θ1θ1'θ2θ2'}

Eigenvalues & Eigenvectors

The eigenvalues and eigenvectors are easily obtained with the help of a TI-89 calculator. First, we consider the A^'s identity matrix,

[λIA]=[λ10083λ23000λ183083λ]

Once we define the A^ matrix, the eigenvalues are determined by using the eigVi() function,

λ1=2i
λ2=2i
λ3=1.1547i
λ4=1.1547i

On the other hand, we use the eigVc() function to find the eigenvectors,

k1=[0.2i0.40.4i0.8]k2=[0.2i0.40.4i0.8]k3=[0.29277i0.338060.58554i0.67621]k4=[0.29277i0.338060.58554i0.67621]

Standard Equation

Now, we plug the eigenvalues and eigenvectors to produce the standar equation,

x_=c1k1_eλ1t+c2k_2eλ2t+c3k3_eλ3t+c4k4_eλ4t
x_=c1[0.2i0.40.4i0.8]e2i+c2[0.2i0.40.4i0.8]e2i+c3[0.29277i0.338060.58554i0.67621]e1.1547i+c4[0.29277i0.338060.58554i0.67621]e1.1547i

Matrix Exponential

The matrix exponential is,

z¯˙=A^z¯=TAT1z¯

where

A=[01008302300001830830],

and

T1=[k1|k2|k3|k4]=[0.2i0.2i0.29277i0.29277i0.40.40.338060.338060.4i0.4i0.58554i0.58554i0.80.80.676210.67621],

so

T=(T1)1=[k1|k2|k3|k4]1=[1.25i0.6250.625i0.31251.25i0.6250.625i0.31250.853913i0.739510.426956i0.3697550.853913i0.739510.426956i0.369755]

Again, we can resort to the TI-89 calculator. As it is mentioned above, the matrix exponential is obtained by typing eigVc(a)^-1*a*eigVc(a), where a is the A^ matrix. Thus,

z¯˙=A^z¯=TAT1z¯=[2i00002i00001.1547i00001.1547i]z¯

So, the exponential matrix becomes,

x_˙=A^x_=T1eA^tTx_=eAtx_

where

eA^t=[e2it0000e2it0000e1.1547it0000e1.1547it]

Hence,

x_˙=[0.2i0.2i0.29277i0.29277i0.40.40.338060.338060.4i0.4i0.58554i0.58554i0.80.80.676210.67621][e2it0000e2it0000e1.1547it0000e1.1547it][1.25i0.6250.625i0.31251.25i0.6250.625i0.31250.853913i0.739510.426956i0.3697550.853913i0.739510.426956i0.369755]