Double Pendulum

A double pendulum system as shown in Fig 1, consists of two-point masses m1m_1 and m2m_2 suspended by strings of length l1l_1 and l2l_2 as shown below. Let the system vibrates in vertical plane with small amplitudes, under which conditions the masses may be considered to have only horizontal motion. Let θ1θ_1 and θ2θ_2 be the angles the strings at any instant make with vertical and let x1x_1 and x2x_2 be the horizontal displacements of the two masses, such that the following relationships holds good for small amplitudes.

sinθ1=θ1=x1l1\sin \theta_1 = \theta_1 = \frac{x_1}{l_1}
sinθ1=θ2=x2x1l2\sin \theta_1 = \theta_2 = \frac{x_2-x_1}{l_2}

For finding natural frequency and mode shapes: Considering no motion in vertical direction, the vertical components of forces on each of two masses must balance. Therefore,

T2=m2gT_2 = m_2g
T1=m1g+T2=(m1m2)gT_1 = m_1g + T_2 = (m_1 - m_2)g

Fig 1. Repesentation of variables in the double pendulum

Fig 2. Free body diagram of the double pendulum

Writing down the equation of motion of two masses for motion in horizontal direction from Fig 2, we have

m1x¨1=T2sinθ2T1sinθ1m_1\ddot{x}_1 = T_2 \sin\theta_2 - T_1 \sin\theta_1
m2x¨2=T2sinθ2m_2\ddot{x}_2 = -T_2 \sin\theta_2

If we take T1T_1 and T2T_2 values in the above equation, we get

m1x¨1+[m1+m2l1+m2l2]gx1=m2l2gx2m_1\ddot{x}_1 + \left[ \frac{m_1+m_2}{l_1} + \frac{m_2}{l_2} \right] gx_1 = \frac{m_2}{l_2} gx_2
m2x¨2+m2l2gx2=m2l2gx1m_2\ddot{x}_2 + \frac{m_2}{l_2} gx_2 = \frac{m_2}{l_2} gx_1

Assuming the general solution of equation of motion to be:

x1=X1sin(ωt)x_1 = X_1 \sin(\omega t)
x2=X2sin(ωt)x_2 = X_2 \sin(\omega t)

Substituting the above solutions with the equation of motion, we get

{m1ω2+[m1+m2l1+m2l2]g}X1=m2l2gX2\left\{ -m_1\omega^2 + \left[ \frac{m_1+m_2}{l_1} + \frac{m_2}{l_2} \right]g \right\} X_1 = \frac{m_2}{l_2} g X_2
{m2ω2+[m2l2]g}X2=m2l2gX1\left\{ -m_2\omega^2 + \left[ \frac{m_2}{l_2} \right]g \right\} X_2 = \frac{m_2}{l_2} g X_1

This equation will give,

X1X2=m2l2gm1ω2+[m1+m2l1+m2l2]g\frac{X_1}{X_2} = \frac{\frac{m_2}{l_2}g}{-m_1\omega^2+\left[\frac{m_1+m_2}{l_1}+\frac{m_2}{l_2}\right]g}
X1X2=m2ω2+[m2l2]gm2l2gX1\frac{X_1}{X_2} = \frac{-m_2\omega^2+\left[\frac{m_2}{l_2}\right]g}{\frac{m_2}{l_2}gX_1}

Equating the two expressions in the above two equations and cross multiplying.

If E=(m2g)/l2E = (m_2 g)/l_2 and F=(m1+m2)g/l1F = (m_1+m_2)g/l_1 , then the frequency equation is

ω4[(m1+m2)E+m2Fm1m2]ω2+FEm1m2=0\omega^4 - [\frac{(m_1+m_2)E + m_2F}{m_1m_2}]\omega^2 + \frac{FE}{m_1m_2} = 0

The above equation is quadratic in ω2\omega^2 and gives two values of ω2\omega^2, and therefore two positive values of ω\omega corresponding to two natural frequencies ωn1\omega_{n1} and ωn2\omega_{n2} of the system. The above equation is called the frequency equation since the roots of this equation gives the natural frequencies of the system. Considering,

m1=m2=mm_1 = m_2 = m
l1=l2=ll_1 = l_2 = l

The above equations become,

X1X2=g/l3glω2\frac{X_1}{X_2} = \frac{g/l}{\frac{3g}{l} - \omega^2}

X1X2=glω2gl\frac{X_1}{X_2} = \frac{\frac{g}{l} - \omega^2}{\frac{g}{l}}

which gives,

g/l3glω2=glω2gl\frac{g/l}{\frac{3g}{l} - \omega^2}=\frac{\frac{g}{l} - \omega^2}{\frac{g}{l}}

or

w4g24w4lg+2l2=0\frac{w^4}{g^2} - \frac{4w^4}{l^g} + \frac{2}{l^2} = 0

which is the frequency equation.

Solving for ω\omega, using quadratic equation we have the two values of the natural frequencies as,

wn1=gl(22)w_{n1} = \sqrt{\frac{g}{l}(2-\sqrt2)}
wn2=gl(2+2)w_{n2} = \sqrt{\frac{g}{l}(2+\sqrt2)}

The amplitude ratio of the equations are:

X1X2=m2l2gm1ω2+[m1+m2l1+m2l2]g\frac{X_1}{X_2} = \frac{\frac{m_2}{l_2} g}{-m_1 \omega^2 + \left[ \frac{m_1 + m_2}{l_1} + \frac{m_2}{l_2} \right] g}

X1X2=m2ω2+[m2l2]gm2l2gX1\frac{X_1}{X_2} = \frac{ -m_2 \omega^2 + \left[ \frac{m_2}{l_2} \right] g }{ \frac{m_2}{l_2} g X_1 }

If in either of the equations, on substituting for ω\omega the value of ωn1\omega_{n1}, we have the first mode shape of the system i.e., when the system is vibrating with the first natural frequency ωn1\omega_{n1}, the mode shape is such that the ratio of the amplitude of two masses is equal to the solution of above equation.

Similarly, in either of the equations, substituting for ω\omega the value of ωn2\omega_{n2}, we have the second mode shape of the system i.e., when the system is vibrating with the second natural frequency ωn2\omega_{n2}, the mode shape is such that the ratio of the amplitude of two masses is equal to the solution of above equation.

For calculating the motion of point masses:

The cartesian co-ordinates of two-point masses in a double pendulum are,

On solving the equations of motion in polar coordinates and we are going to use the Lagrangian method (L=TVL=T-V where TT is kinetic energy of system and VV is potential energy of system) to derive them.

The kinetic energy of the system:

T=12m1v12+12m2v22T = \frac{1}{2} m_1 v_1^2 + \frac{1}{2} m_2 v_2^2

T=12m1(x˙12+y˙12)+12m2(x˙22+y˙22)T = \frac{1}{2} m_1 (\dot{x}_1^2 + \dot{y}_1^2) + \frac{1}{2} m_2 (\dot{x}_2^2 + \dot{y}_2^2)

T=12m1l12θ˙12+12m2[l12θ˙12+l22θ˙22+2l1l2θ˙1θ˙2cos(θ1θ2)]T = \frac{1}{2} m_1 l_1^2 \dot{\theta}_1^2 + \frac{1}{2} m_2 \left[ l_1^2 \dot{\theta}_1^2 + l_2^2 \dot{\theta}_2^2 + 2 l_1 l_2 \dot{\theta}_1 \dot{\theta}_2 \cos(\theta_1 - \theta_2) \right]

The potential energy of system:

V=m1gy1+m2gy2V = m_1 g y_1 + m_2 g y_2

V=(m1+m2)gl1cosθ1m2gl2cosθ2V = - (m_1 + m_2) g l_1 \cos\theta_1 - m_2 g l_2 \cos\theta_2

The Lagrange equations for θ1\theta_1 and θ2\theta_2 are,

ddt(dLdθ˙l)dLdθl=0\frac{d}{dt} \left( \frac{d L}{d \dot{\theta}_l} \right) - \frac{d L}{d \theta_l} = 0

On solving,

θ¨1=g(sinθ2cos(θ1θ2)μsinθ1)(l2θ˙22+l1θ˙12cos(θ1θ2))sin(θ1θ2)l1(μcos2(θ1θ2))\ddot{\theta}_1 = \frac{g(\sin\theta_2 \cos(\theta_1 - \theta_2) - \mu \sin\theta_1) - (l_2 \dot{\theta}_2^2 + l_1 \dot{\theta}_1^2 \cos(\theta_1 - \theta_2)) \sin(\theta_1 - \theta_2)}{l_1 (\mu - \cos^2(\theta_1 - \theta_2))}

θ¨2=gμ(sinθ1cos(θ1θ2)sinθ2)(μl1θ˙12+l2θ˙22cos(θ1θ2))sin(θ1θ2)l2(μcos2(θ1θ2))\ddot{\theta}_2 = \frac{g \mu (\sin\theta_1 \cos(\theta_1 - \theta_2) - \sin\theta_2) - (\mu l_1 \dot{\theta}_1^2 + l_2 \dot{\theta}_2^2 \cos(\theta_1 - \theta_2)) \sin(\theta_1 - \theta_2)}{l_2 (\mu - \cos^2(\theta_1 - \theta_2))}

Where μ=1+(m1+m2)\mu = 1 + (m_1 + m_2), θ¨1 \ddot θ1 and θ¨2 \ddot θ2 are angular accelerations of point masses m1m_1 and m2m_2 and θ˙1 \dot θ1 and θ˙2 \dot θ2 are angular velocities of point masses m1m_1 and m2m_2.