What Is the Next Step in Simplifying the Van der Pol Oscillator Equation?

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SUMMARY

The discussion focuses on simplifying the Van der Pol oscillator equation, specifically for the case when ##\epsilon = 0##. The limit cycle is established as circular in phase space, with the Fourier series representation given by ##x_\epsilon^p(t) = \frac{a_0}{2} + \sum\limits_{k=1}^{\infty } [a_k \cos(k \omega t) + b_k \sin(k \omega t)]##. The participants conclude that the next steps involve utilizing trigonometric identities to further simplify the equation of motion, which is expressed as $$\ddot{x} + \epsilon(x^{2} - 1)\dot{x} + x = 0$$. The goal is to derive the equation $$\epsilon (x_p^2 - 1)\dot{x_p} = \epsilon a_1\omega[(1-\frac{a_1^2}{4})\sin(\omega t)-\frac{a_1^2}{4}\sin(3 \omega t)]$$.

PREREQUISITES
  • Understanding of Van der Pol oscillator dynamics
  • Familiarity with Fourier series and their applications
  • Knowledge of trigonometric identities and their manipulation
  • Basic differential equations, particularly second-order linear equations
NEXT STEPS
  • Explore the derivation of the Van der Pol oscillator limit cycle using phase space analysis
  • Study the application of Fourier series in solving differential equations
  • Investigate the use of trigonometric identities in simplifying nonlinear equations
  • Learn about perturbation methods for analyzing small parameter effects in differential equations
USEFUL FOR

Mathematicians, physicists, and engineers interested in dynamical systems, particularly those working with oscillatory systems and nonlinear differential equations.

kornelthefirst
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Homework Statement
We have a Van der Pol oscillator with small ##\epsilon## and after writing up a Fourier-series we have to bring it to a simpler form.
Relevant Equations
Equation of motion for the Van der Pol oscillator$$\ddot{x} + \epsilon(x^{2} - 1)\dot{x} + x = 0$$ Fourier-series for the limit cycle(already given) $$x_\epsilon^p(t) = \frac{a_0}{2} + \sum\limits_{k=1}^{\infty } [a_k \cos(k \omega t) + b_k \sin(k \omega t)]$$ Equation we need to arrive to$$\epsilon (x_p^2 - 1)\dot{x_p} = \epsilon a_1\omega[(1-\frac{a_1^2}{4})\sin(\omega t)-\frac{a_1^2}{4}\sin(3 \omega t)]$$
First i looked at the case of ## \epsilon = 0## and came to the conclusion, that this oscillator has a circular limit cycle in a phase space trajectory, when plotted with the axes x and ##\dot{x}##.
I have found that ##x_0^p (t) = a_1 \cos(t)## which implies that all other Fourier- coefficients have ##\epsilon## of at least power of 1
The limit cycle is independent of the starting conditions unless ##x = 0## and ##\dot{x} = 0##, so we can choose ##a_1## to be > 0 and ##b_1 > 0##.
If we put the equation of the Fourier-series back to the equation of motion we get$$\sum\limits_{k=1}^{\infty } [ - a_k \cos(k \omega t) - b_k sin( k \omega t)] + \epsilon (x^2-1)\dot{x} + \frac{a_0}{2}+\sum\limits_{k=1}^{\infty } [a_k \cos(k \omega t) + b_k sin( k \omega t)]$$ so simplified $$\epsilon (x^2-1)\dot{x} + \frac{a_0}{2} = 0$$ I am currently stuck here and can't find the next step. I can only assume it will include trigonometric identities, because i can see some patterns for some.
 
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kornelthefirst said:
Homework Statement: We have a Van der Pol oscillator with small ##\epsilon## and after writing up a Fourier-series we have to bring it to a simpler form.

I'm not sure this is the best approach to this problem; could you please post the exact problem statement?

Relevant Equations: Equation of motion for the Van der Pol oscillator$$\ddot{x} + \epsilon(x^{2} - 1)\dot{x} + x = 0$$ Fourier-series for the limit cycle(already given) $$x_\epsilon^p(t) = \frac{a_0}{2} + \sum\limits_{k=1}^{\infty } [a_k \cos(k \omega t) + b_k \sin(k \omega t)]$$ Equation we need to arrive to$$\epsilon (x_p^2 - 1)\dot{x_p} = \epsilon a_1\omega[(1-\frac{a_1^2}{4})\sin(\omega t)-\frac{a_1^2}{4}\sin(3 \omega t)]$$

First i looked at the case of ## \epsilon = 0## and came to the conclusion, that this oscillator has a circular limit cycle in a phase space trajectory, when plotted with the axes x and ##\dot{x}##.
I have found that ##x_0^p (t) = a_1 \cos(t)## which implies that all other Fourier- coefficients have ##\epsilon## of at least power of 1
The limit cycle is independent of the starting conditions unless ##x = 0## and ##\dot{x} = 0##, so we can choose ##a_1## to be > 0 and ##b_1 > 0##.
If we put the equation of the Fourier-series back to the equation of motion we get$$\sum\limits_{k=1}^{\infty } [ - a_k \cos(k \omega t) - b_k sin( k \omega t)] + \epsilon (x^2-1)\dot{x} + \frac{a_0}{2}+\sum\limits_{k=1}^{\infty } [a_k \cos(k \omega t) + b_k sin( k \omega t)]$$

You should have <br /> \ddot x = -\sum_{n=1}^\infty n^2\omega^2 (a_n \cos (n\omega t) + b_n \sin (n\omega t)).

I am currently stuck here and can't find the next step. I can only assume it will include trigonometric identities, because i can see some patterns for some.

I think the idea is that x(t) = a_1 \cos \omega t + \epsilon x_p(t) so that \begin{split}<br /> \ddot x + x &amp;= -\epsilon(x^2 - 1)\dot x \\<br /> (1 - \omega^2) \cos \omega t + \epsilon (\ddot x_p + x_p) &amp;= \epsilon a_1 \omega (a_1^2 \cos^2\omega t - 1)\sin \omega t + O(\epsilon^2)\end{split} subject to \dot x_p(0) = x_p(0) = 0. We do not need a sine term in the leading order solution since that just amounts to a shift in the origin of time, which merely moves us to a different point on the limit cycle. It is not necessary to expand x_p as a fourier series in order to solve this, although expressing the right hand side as a series in \sin n\omega t and knowing \ddot y + y where y = \sin n\omega t or t\cos n\omega t will assist.
 

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