Elementary pendulum equation of motion

AI Thread Summary
The discussion focuses on deriving the equation of motion for a pendulum using conservation of energy rather than Newton's laws. The initial approach involved setting up equations for kinetic and potential energy at different points of the pendulum's swing, but it led to an incorrect non-periodic solution. Participants emphasized the need for an equation that relates angular displacement and angular velocity at the same point in the motion, rather than at different points. The correct method involves equating energy states to derive a function for angular displacement over time, with a suggestion to apply the small angle approximation to simplify the calculations. The conversation highlights the importance of maintaining consistency in the equations used for accurate modeling of the pendulum's motion.
jonjacson
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Homework Statement


To find the period of oscillation of the pendulum and the equation of motion.

Homework Equations


Conservation of energy.
Potential energy in a constant field = mgh.
Kinetic energy in polar coordinates with r constant = (1/2) m r2 (dΘ2/dt2)

The Attempt at a Solution


I won't use the Newton laws because that means a second order differential equation. Instead I use the conservation of energy so I start from a first order equation.

1.- I set the origin of coordinates at the anchor point of the pendulum.
2.- I will use polar coordinates, the angle starts counting from the vertical counterclockwise.
3.- The energy is conserved so at the point 1 (at the bottom when the pendulum is faster) we have:
L is the length of the pendulum

KE =(1/2) mL22/dt2

Potential energy = -mgL ; I set the potential energy as zero at the origin of coordinates, the anchor point of the pendulum.

At the point 2 when the speed is zero I have:

KE = 0

PE = -mg (lcosΘ)

Now I equate the sum of the KE and PE at both points:

(1/2)mL22/dt2 -mgL = 0 -mg (LcosΘ)

(1/2) dΘ2/dt2 = g(1 - cos Θ ) /L

If Θ is small cos Θ can be aproximated by 1 - Θ2/2, so:

(1/2) dΘ2/dt2 = g ( 1- (1-Θ2/2))/L

Finally:

dΘ/dt = √(g/L) Θ2

dΘ/√(g/L) Θ2 = dt

Since Θ can get outside de square the integral is :

Log Θ = √L/g t + constant

And the basic expression is an exponential:

So Θ= exp t

And this is not the expected periodic movement and that does not make any sense. Does anybody know where is the mistake?

THanks

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You need an equation that holds at each point of the motion rather than an equation that just relates the lowest and highest points of the motion. Your equation relates dΘ/dt at one point to Θ at another point. Instead, try to get an equation that relates dΘ/dt and Θ at the same point.
 
TSny said:
You need an equation that holds at each point of the motion rather than an equation that just relates the lowest and highest points of the motion.

But shouldn't this be equivalent?

I mean, if I differenciate my equation, SHouldn't I get the Newton equations?
 
If you were to add subscripts 1 and 2 to denote the two points that you selected, you have an equation that involves [dΘ/dt]2 and Θ1 . So, you aren't getting a differential equation that holds throughout the motion.
 
TSny said:
If you were to add subscripts 1 and 2 to denote the two points that you selected, you have an equation that involves [dΘ/dt]2 and Θ1 . So, you aren't getting a differential equation that holds throughout the motion.

Ok I understand, so basically what I did simply didn't make sense.

THe equation could have been used to find only differences between energies, and nothing else.
 
So it could be calculated this way:

(1/2) m L2 (dΘ/dt)2 - mgL cos Θ= -mgL cos Θ0

Θ0 is the maximum angle.
Θ is a function of time

It means, the energy at an arbitrary point equals the maximum energy at the top of the movement.

From this it should be possible to obtain Θ(t) right?
 
Yes. Good.
 
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Are you going to make a small angle approximation soon. Otherwise, you will end up with an elliptic integral.
 
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