Double Pendulum

In physics and mathematics, in the area of dynamical systems, a double pendulum also known as a chaos pendulum is a pendulum with another pendulum attached to its end, forming a simple physical system that exhibits rich dynamic behavior with a strong sensitivity to initial conditions. The motion of a double pendulum is governed by a set of coupled ordinary differential equations and is chaotic.

Analysis and interpretation

Several variants of the double pendulum may be considered; the two limbs may be of equal or unequal lengths and masses, they may be simple pendulums or compound pendulums (also called complex pendulums) and the motion may be in three dimensions or restricted to the vertical plane. In the following analysis, the limbs are taken to be identical compound pendulums of length and mass , and the motion is restricted to two dimensions.

In a compound pendulum, the mass is distributed along its length. If the mass is evenly distributed, then the center of mass of each limb is at its midpoint, and the limb has a moment of inertia of about that point.

It is convenient to use the angles between each limb and the vertical as the generalized coordinates defining the configuration of the system. These angles are denoted and . The position of the center of mass of each rod may be written in terms of these two coordinates. If the origin of the Cartesian coordinate system is taken to be at the point of suspension of the first pendulum, then the center of mass of this pendulum is at:
:$\begin x_1 &= \frac \sin \theta_1 \\ y_1 &= -\frac \cos \theta_1 \end$
and the center of mass of the second pendulum is at
:$\begin x_2 &= l \left ( \sin \theta_1 + \tfrac \sin \theta_2 \right ) \\ y_2 &= -l \left ( \cos \theta_1 + \tfrac \cos \theta_2 \right ) \end$
This is enough information to write out the Lagrangian.

Lagrangian

The Lagrangian is
:$\beginL & = \text - \text \\ & = \tfrac m \left ( v_1^2 + v_2^2 \right ) + \tfrac I \left ( ^2 + ^2 \right ) - m g \left ( y_1 + y_2 \right ) \\ & = \tfrac m \left ( ^2 + ^2 + ^2 + ^2 \right ) + \tfrac I \left ( ^2 + ^2 \right ) - m g \left ( y_1 + y_2 \right ) \end$
The first term is the ''linear'' kinetic energy of the center of mass of the bodies and the second term is the ''rotational'' kinetic energy around the center of mass of each rod. The last term is the potential energy of the bodies in a uniform gravitational field. The dot-notation indicates the time derivative of the variable in question.

Substituting the coordinates above and rearranging the equation gives
:$L = \tfrac m l^2 \left ( ^2 + 4 ^2 + 3 \cos (\theta_1-\theta_2) \right ) + \tfrac m g l \left ( 3 \cos \theta_1 + \cos \theta_2 \right ).$
There is only one conserved quantity (the energy), and no conserved momenta. The two generalized momenta may be written as

:$\begin p_ &= \frac = \tfrac m l^2 \left ( 8 + 3 \cos (\theta_1-\theta_2) \right ) \\ p_ &= \frac = \tfrac m l^2 \left ( 2 + 3 \cos (\theta_1-\theta_2) \right ). \end$

These expressions may be inverted to get

:$\begin &= \frac \frac \\ &= \frac \frac. \end$

The remaining equations of motion are written as

:$\begin &= \frac = -\tfrac m l^2 \left ( \sin (\theta_1-\theta_2) + 3 \frac \sin \theta_1 \right ) \\ &= \frac = -\tfrac m l^2 \left ( - \sin (\theta_1-\theta_2) + \frac \sin \theta_2 \right ). \end$

These last four equations are explicit formulas for the time evolution of the system given its current state. It is not possible to go further and integrate these equations to an expression in closed form, to get formulas for and as functions of time. It is, however, possible to perform this integration numerically using the Runge Kutta method or similar techniques.

Chaotic motion

The double pendulum undergoes chaotic motion, and shows a sensitive dependence on initial conditions. The image to the right shows the amount of elapsed time before the pendulum flips over, as a function of initial position when released at rest. Here, the initial value of ranges along the -direction from −3.14 to 3.14. The initial value ranges along the -direction, from −3.14 to 3.14. The colour of each pixel indicates whether either pendulum flips within:
* $\sqrt$ (black)
* $10\sqrt$ (red)
* $100\sqrt$ (green)
* $1000\sqrt$ (blue) or
* $10000\sqrt$ (purple).

Initial conditions that do not lead to a flip within $10000\sqrt$ are plotted white.

The boundary of the central white region is defined in part by energy conservation with the following curve:

:$3 \cos \theta_1 + \cos \theta_2 = 2.$

Within the region defined by this curve, that is if

:$3 \cos \theta_1 + \cos \theta_2 > 2,$

then it is energetically impossible for either pendulum to flip. Outside this region, the pendulum can flip, but it is a complex question to determine when it will flip. Similar behavior is observed for a double pendulum composed of two point masses rather than two rods with distributed mass.Alex Small,
Sample Final Project: One Signature of Chaos in the Double Pendulum
', (2013). A report produced as an example for students. Includes a derivation of the equations of motion, and a comparison between the double pendulum with 2 point masses and the double pendulum with 2 rods.

The lack of a natural excitation frequency has led to the use of double pendulum systems in seismic resistance designs in buildings, where the building itself is the primary inverted pendulum, and a secondary mass is connected to complete the double pendulum.

See also

* Double inverted pendulum
* Pendulum (mechanics)
* Mid-20th century physics textbooks use the term "double pendulum" to mean a single bob suspended from a string which is in turn suspended from a V-shaped string. This type of pendulum, which produces Lissajous curves, is now referred to as a Blackburn pendulum.

Notes

References

*
* Eric W. Weisstein,
Double pendulum
' (2005), ScienceWorld ''(contains details of the complicated equations involved)'' and
Double Pendulum
by Rob Morris, Wolfram Demonstrations Project, 2007 (animations of those equations).
* Peter Lynch,
Double Pendulum
', (2001). ''(Java applet simulation.)''
* Northwestern University,

'', ''(Java applet simulation.)''
* Theoretical High-Energy Astrophysics Group at UBC,
Double pendulum
', (2005).

External links

*Animations and explanations of
double pendulum
and
physical double pendulum (two square plates)
by Mike Wheatland (Univ. Sydney)

*Interactive Open Source Physics JavaScript simulation with detailed equation
double pendulum
*Interactive Javascript simulation of

*Double pendulum physics simulation fro

usin
open source JavaScript code
*Simulation, equations and explanation o
Rott's pendulum
*

Double Pendulum Simulator
- An open source simulator written in C++ using the Qt toolkit.

Online Java simulator
of the Imaginary exhibition.

{{Chaos theory

Chaotic maps
Dynamical systems
Mathematical physics
Pendulums