Mathematical model of pendulum

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SUMMARY

The mathematical model of an ideal pendulum is defined by the equation L \ddot{\theta} + g sin \theta = 0, where L represents the pendulum length and g is the acceleration due to gravity. The total energy per unit mass of the pendulum is expressed as E(\theta,\dot{\theta}) = \frac{1}{2}L \dot{\theta}^2 - g cos \theta. It is established that this energy remains constant over time, leading to the conclusion that \frac{1}{2}L\dot{\theta}^2 - g cos \theta + g cos \theta_0 = 0 holds true for all t ≥ 0, confirming the conservation of energy in the system.

PREREQUISITES
  • Understanding of classical mechanics, specifically pendulum motion.
  • Familiarity with differential equations and their applications in physics.
  • Knowledge of energy conservation principles in mechanical systems.
  • Ability to differentiate functions with respect to time.
NEXT STEPS
  • Study the derivation of the equations of motion for pendulums using Lagrangian mechanics.
  • Explore the implications of energy conservation in non-linear pendulum systems.
  • Learn about numerical methods for solving differential equations related to pendulum dynamics.
  • Investigate the effects of damping and external forces on pendulum motion.
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limofunder
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Homework Statement

W
We know the model of an ideal pendulum at rest is given by
L \ddot{\theta} + g sin \theta =0, t\geq0
\dot{\theta}(0)=0
\theta(0)=\theta_0
where \theta(t) is the pendulum angle at time t, L is the length of the pendulum, and g is gravity.
Now, consider the total energy per unit mass of the pendulum given by
E(\theta,\dot{\theta}) = \frac{1}{2}L \dot{\theta}^2 - g cos \theta
Show that this equation is constant along the previously given solutions (the first 3 equations initially given, let's call them EQ [1] ), \forall t\geq0. Use this result to show that the solution of [1] should satisfy
\frac{1}{2}L\dot{\theta}^2-g cos \theta + g cos \theta_0 = 0, \forall t\geq0
(lets call this EQN [2])

Homework Equations



we know that if E(theta, thetadot) is a constant, then
\frac{d E(\theta,\dot{\theta})}{dt} = 0

The Attempt at a Solution


so, taking the derivative of the energy, we have:

\frac{d E(\theta,\dot{\theta})}{dt} = \frac{d}{dt}[\frac{1}{2} L \dot{\theta}^2 - g cos \theta]

= L \ddot{\theta} +\dot{\theta}g sin\theta
however, this does not seem to equal [1], as \dot{\theta}gsin\theta never appears in the solution. what am I doing wrong?
or do we not take the time derivative of the second term in the energy equation (the sin(theta) term), thus giving
\frac{d E(\theta,\dot{\theta})}{dt} =L \ddot{\theta} +g sin\theta which is equal to zero by definition of [1], thus if the derivative of the energy equation is equal to zero, then by definition of constant, energy is constant!
now, i am in confusion as how to use this result to prove EQN [2]?
 
Last edited:
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Hi limofunder! :smile:

(have a theta: θ :wink:)
limofunder said:
\frac{d E(\theta,\dot{\theta})}{dt} = \frac{d}{dt}[\frac{1}{2} L \dot{\theta}^2 - g cos \theta]

= L \ddot{\theta} +\dot{\theta}g sin\theta

hmm :rolleyes: … d/dt (Lθ') = Lθ''

but d/dt (Lθ'2) = … ? :smile:
 
limofunder said:
\frac{d E(\theta,\dot{\theta})}{dt} = \frac{d}{dt}[\frac{1}{2} L \dot{\theta}^2 - g cos \theta]

= L \ddot{\theta} +\dot{\theta}g sin\theta

\frac{d}{dt}\left(\frac{1}{2} L \dot{\theta}^2\right)=L\dot{\theta}\ddot{\theta}

:wink:

EDIT: Tinytim beat me to it
 
ok, so then that gives way to
dE/dt = θ' (Lθ''+g sinθ)
the second term being by definition of [1] >= 0 for all time.
Thank you,
so that still begs the question, I do not see how this forces
[1] to satisfy
1/2 Lθ' - g cosθ + g cosθ0
 
limofunder said:
ok, so then that gives way to
dE/dt = θ' (Lθ''+g sinθ)
the second term being by definition of [1] >= 0 for all time.
Thank you,
so that still begs the question, I do not see how this forces
[1] to satisfy
1/2 Lθ' - g cosθ + g cosθ0

Because E = constant is a solution, so just call the constant gcosθ0 :smile:
 

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