## Dubby Pendy — A Double Pendulum Simulator

### Chaos is interesting, and visualising it is important.

Learning about Lagrangian and Hamiltonian mechanics introduced me to an entirely new way of solving physics problems. The first time I’d read about this topic was in The Principle of Least Action chapter in Vol. 2 of The Feynman Lectures on Physics. I was introduced to a different perspective of viewing the physical world, perhaps a more general one than Newton’s laws.

A famous example of a system whose equations of motion can be more easily attained using Lagrangian or Hamiltonian mechanics is the double pendulum. I saw a Wolfram Science animation of the system, but it didn’t have the right a e s t h e t i c for me, and I wanted to write one of my own to investigate the system for various initial conditions and its chaotic behaviour.

The following shows the double pendulum system: The Lagrangian of the system is:

\mathcal{L} = T - V \quad \mathrm{where} \quad \begin{aligned} 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 + 2l_1 l_2 \dot{\theta}_1 \dot{\theta}_2 \cos(\theta_1 - \theta_2)\right] \\ V & = -(m_1 + m_2)gl_1\cos \theta_1 - m_2gl_2\cos\theta_2 \end{aligned}

After a very long and painful derivation, Hamilton’s equations can be obtained:

\begin{aligned} \dot{\theta_1} & = \frac{l_2 p_{\theta_1} - l_1 p_{\theta_2}\cos(\theta_1 - \theta_2)}{l_1^2 l_2[m_1 + m_2\sin^2(\theta_1-\theta_2)]} \\ \dot{\theta_2} & = \frac{l_1 (m_1 + m_2)p_{\theta_1} - l_2 m_2 p_{\theta_1}\cos(\theta_1 - \theta_2)}{l_1 l_2^2 m_2[m_1 + m_2\sin^2(\theta_1-\theta_2)]} \\ \dot{p}_{\theta_1} & = -(m_1 + m_2)gl_1\sin\theta_1 - C_1 + C_2 \\ \dot{p}_{\theta_2} & = -m_2gl_2\sin\theta_2 + C_1 - C_2 \\ C_1 & = \frac{p_{\theta_1}p_{\theta_2}\sin(\theta_1-\theta_2)}{l_1 l_2[m_1 + m_2\sin^2(\theta_1-\theta_2)]} \\ C_2 & = \frac{l_2^2 m_2 p_{\theta_1}^2 + l_1^2(m_1 + m_2)p_{\theta_2}^2 - l_1 l_2 m_2 p_{\theta_1} p_{\theta_2} \cos(\theta_1 - \theta_2)}{2l_1^2 l_2^2 [m_1 + m_2\sin^2(\theta_1-\theta_2)]^2}\sin[2(\theta_1 - \theta_2)] \end{aligned}

These are very formidable-looking equations, and it is almost impossible to determine the particle trajectories by solving these equations analytically! So how does one solve it for practical purposes? Numerical methods and programming. I used Lua to program the simulator, including the LÖVE framework for the graphics.

Since the only data structure in Lua is a table, I decided to see how I could make use of that property for this program. Lua doesn’t have functions to perform scalar multiplication or addition between tables, so I wrote some:

function directSum(a, b)
local c = {}
for i,v in pairs(a) do
c[i] = a[i] + b[i]
end
return c
end

function scalarMultiply(scalar, table)
local output = {}
for i,v in pairs(table) do
output[i] = scalar*table[i]
end
return output
end


So now I can store values, such as the initial conditions and parameters of the system in a table and perform basic arithmetic operations between tables to change values. Now to implement the physics of the problem.

First, I defined a generator that randomly generates initial values (within a given range) of the masses of the bobs, the lengths of the rods, their angles with respect to the vertical, their initial angular velocities and calculated the momenta of the bobs. This is fed into a table called data:

function Generator()

local self = {}

self.m1 = love.math.random( 3, 10 )
self.m2 = love.math.random( 3, 10 )
self.l1 = love.math.random( 3, 10 )
self.l2 = love.math.random( 1, 10 )
self.t1 = love.math.random( -6.28, 6.28 )
self.t2 = love.math.random( -6.28, 6.28 )
self.o1 = love.math.random( -4, 4 )
self.o2 = love.math.random( -2, 2 )
self.p1 = (self.m1+self.m2)*(math.pow(self.l1, 2))*self.o1
+ self.m2*self.l1*self.l2*self.o2*math.cos(self.t1-self.t2)
self.p2 = self.m2*(math.pow(self.l2, 2))*self.o2
+ self.m2*self.l1*self.l2*self.o1*math.cos(self.t1-self.t2)

return self
end

data = Generator()


Now we set up the equations of motion using a function called Hamiltonian. It takes the initial values from data to perform calculations, and a new table called phase which consists of the phase space variables to update the angles and momenta over time:

function Hamiltonian(phase, data)

local update = {}

t1 = phase
t2 = phase
p1 = phase
p2 = phase

C0 = data.l1*data.l2*(data.m1+data.m2*math.pow(math.sin(t1-t2),2))
C1 = (p1*p2*math.sin(t1-t2))/C0
C2 = (data.m2*(math.pow(data.l2*p1,2))+(data.m1+data.m2)*
(math.pow(data.l1*p2, 2))-2*data.l1*data.l2*data.m2*p1*p2*
math.cos(t1-t2))*math.sin(2*(t1-t2))/(2*(math.pow(C0,2)))

update = (data.l2*p1 - data.l1*p2*math.cos(t1-t2)) / (data.l1*C0)
update = (data.l1*(data.m1+data.m2)*p2 - data.l2*data.m2*p1*
math.cos(t1-t2)) / (data.l2*data.m2*C0)
update = -(data.m1 + data.m2)*g*data.l1*math.sin(t1) - C1 + C2
update = -data.m2*g*data.l2*math.sin(t2) + C1 - C2

return update
end


All the required information with regard to the physics are now processed. To solve the differential equations, I implemented the Runge-Kutta method of order 4, performing operations on the tables using directSum and scalarMultiply. These operations take place in Solver, which takes the time input dt from LÖVE in love.update().

function Solver(dt)

local phase = {data.t1, data.t2, data.p1, data.p2}

local k1 = Hamiltonian(phase, data)
local k2 = Hamiltonian(directSum(phase, scalarMultiply(dt/2, k1)), data)
local k3 = Hamiltonian(directSum(phase, scalarMultiply(dt/2, k2)), data)
local k4 = Hamiltonian(directSum(phase, scalarMultiply(dt, k3)), data)

local R = scalarMultiply(1/6 * dt,
directSum(directSum(k1, scalarMultiply(2.0, k2)),
directSum(scalarMultiply(2.0, k3), k4)))

data.t1 = data.t1 + R
data.t2 = data.t2 + R
data.p1 = data.p1 + R
data.p2 = data.p2 + R
end

function love.update()
Solver(dt)
end


After setting up the graphics end, I obtain nice animations like this:

I’ll probably end up creating a new post with cool patterns emerging from this simulation, possibly checking for chaotic behaviour with initial conditions that are not so different from a previous state.

Licensed under CC BY-NC-SA 4.0