Pendulum - Stability and fixed points

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The discussion focuses on analyzing the dynamics of a pendulum using Lagrangian mechanics and phase space. It begins with demonstrating the Lagrangian derivative and how phase space evolves over time, indicating that the system converges to an attractor when the rate of flow is positive. Fixed points are identified at integer multiples of π, with even multiples being stable attractors and odd multiples being unstable saddle points. Further analysis reveals that fixed points depend on the relationship between parameters, with stability determined by the eigenvalues of the system. The final part raises a question about the transition from fixed points to limit cycles when the parameter T exceeds ga, highlighting a gap in understanding this behavior.
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Homework Statement



(a): Show the lagrangian derivative in phase space
(b)i: Show how the phase space evolves over time and how they converge
(b)ii: Find the fixed points and stability and sketch phase diagram
(c)i: Find fixed points and stability
(c)ii: Show stable limit cycles exist for T>ga and why they cannot emerge by hopf bifurcations[/B]

2vtqfcz.png

Homework Equations

The Attempt at a Solution



Part(a)
[/B]
Shown using conservation of rate of flow of mass.

Part(b)i

\Delta \dot V = \Delta V \left( \frac{\partial \dot \theta}{\partial \theta} + \frac{\partial \dot \omega}{\partial \omega} \right)
\Delta \dot V = -r \Delta V

\Delta V = \Delta V_0 e^{-rt}

Thus for ##r>0## system converges to an attractor.

Part (b)ii
For ## \dot \omega = \dot \theta = 0##, fixed points are given by ##\theta_0 = n\pi##.

To find their stability, we find ##|J-\lambda I| = 0##
\lambda^2 + \lambda r + ga cos\theta = 0
Thus for even ##n##, fixed points are stable attractors and for odd ##n##, fixed points are unstable saddle points.

1213bjo.png
Part (c)i

Fixed points are given by:

cos \theta = \sqrt{1- \left( \frac{T}{ga} \right)^2}

For their stability, again we find the eigenvalues:

\lambda^2 + \lambda r + ga cos\theta = 0
\lambda = \frac{-r \pm \sqrt{ r^2 - 4ga cos\theta } }{2}

Thus for ## r^2 > 4ga \sqrt{1- \left( \frac{T}{ga} \right)^2}##, they are fixed stable attractors. For ## r^2 < \sqrt{1- \left( \frac{T}{ga} \right)^2} ##, they are unstable saddle points.

Part(c)ii

I'm not too sure about this part. I know that for ##T>ga##, ##cos \theta## becomes imaginary. How do I relate that to how the fixed point changes to a limit cycle?
 
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