Approximate solutions to Kuramoto synchronization model

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SUMMARY

The discussion focuses on the Kuramoto synchronization model, specifically the case of two oscillators governed by the equations $$\frac{d \theta_1}{dt} = \omega_i + \frac{K}{2}\sin(\theta_2 - \theta_1)$$ and $$\frac{d \theta_2}{dt} = \omega_i + \frac{K}{2}\sin(\theta_1 - \theta_2)$$. A transformation using $$re^{i \psi} = \frac{1}{2}(e^{i \theta_1} + e^{i \theta_2})$$ is proposed to simplify the equations. The assumption that the average phase $$\psi$$ is zero is debated, with suggestions to transform angular variables to maintain this condition. The discussion concludes that looking for stationary solutions and expanding in phase space is a viable method for analyzing the system.

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  • Understanding of the Kuramoto model and its governing equations
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Mathematicians, physicists, and engineers interested in synchronization phenomena, particularly those working with the Kuramoto model and non-linear dynamical systems.

Danny Boy
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According to the wiki entry 'Kuramoto Model', if we consider the ##N=2## case then the governing equations are $$\frac{d \theta_1}{dt} = \omega_i + \frac{K}{2}\sin(\theta_2 - \theta_1)~~~\text{and}~~~\frac{d \theta_2}{dt} = \omega_i + \frac{K}{2}\sin(\theta_1 - \theta_2),$$
where ##\theta_i## are the phases of the oscillator, ##\omega_i## are the natural frequencies and $K$ is the coupling constant.

To find solutions I then propose (as in the wiki entry) using the transformation ##re^{i \psi} = \frac{1}{2}(e^{i \theta_1} + e^{i \theta_2})##. Thus allowing us to rewrite the coupled equations as $$\frac{d \theta_i}{dt} = \omega_i + Kr\sin(\psi - \theta_i)~~~~~~~\text{for }i = 1,2~~~~~~~~(1)$$
If we further assume the statistical averages of phases is zero (i.e. ##\psi = 0##), the governing equations then become $$\frac{d \theta_i}{dt} = \omega_i -Kr \sin(\theta_i).~~~~~~~~~~~~~~~~~~(2)$$

Questions:

- Am I correct in stating that ##\psi=0## assumption is quite limiting in that as ##\psi## is also a function of time ##t##, hence even if ##\psi(0) = 0## it does not necessarily imply that ##\psi(t) = 0##?

- What would be a feasible recommended approximation method to attempt to solve the type of ODE in (1)?

Thanks for any assistance.
 
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Yes, setting ##\psi(t)=0## without any other changes seems pretty limiting to me. However, I think it might be more reasonable to transform all of the angular variables (i.e., the ##\theta_i##'s and ##\psi##) in such a way that they all start at zero, and such that the sum/average of the ##\omega_i##'s is zero. Since ##\psi## is sort of an average of the angular variables, ##\psi(t)=0## might not be such a bad approximation after such a transformation.

I think that looking for stationary solutions and then expanding about them in configuration or phase space is typically a good way to gain some information on the behavior of a non-linear system of ODEs.
 
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@IsometricPion Thanks for your response and recommendations. I think the ##\psi(t) = 0## follows from transforming into a rotating reference frame where it rotates such that the average phase is always zero. Hence I think part of my misunderstanding was that I was still thinking in terms of the non-rotating inertial reference frame. It is interesting how little the equations change after the transformation into a rotating reference frame (it goes from ##\frac{d \theta_i}{dt} = \omega_i + Kr\sin(\psi - \theta_i)## to ##\frac{d \theta_i}{dt} = \omega_i -Kr \sin(\theta_i)##).
 

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