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Weak nonlinearity and separation of time scales

Consider weakly nonlinear dispersive waves in a periodic box. Here we consider quadratic nonlinearity and the linear dispersion relations $\omega_k$ which allow three-wave interactions. Example of such systems include surface capillary waves [5,], Rossby waves [13] and internal waves in the ocean [14]. In Fourier space, we have the following Hamiltonian equations,

$\displaystyle i \, \dot a_l$ $\textstyle =$ $\displaystyle \epsilon \sum_{m,n=1}^\infty \left(
V^l_{mn} a_{m} a_{n}e^{i\omeg...
...ar{V}^{m}_{ln} \bar a_{n}
a_{m} e^{-i\omega^m_{ln}t } \, \delta^m_{l+n}\right),$ (7)

where $a_l=a(k_l)$ is the complex wave amplitude in the interaction representation, $k_l = 2
\pi l /L$ is the wavevector, $L$ is the box side length, $\omega^l_{mn}\equiv\omega_{k_l}-\omega_{k_m}-\omega_{k_m}$, $\omega_l=\omega_{k_l}$ is the wave frequency, $V^l_{mn}$ is an interaction coefficient and $\epsilon$ is a formal small nonlinearity parameter.

In order to filter out fast oscillations at the wave period, let us seek for the solution at time $T$ such that $2 \pi / \omega \ll
T \ll 1/\omega \epsilon^2$. The second condition ensures that $T$ is a lot less than the nonlinear evolution time. Now let us use a perturbation expansion in small $\epsilon$,

\begin{displaymath}a_l(T)=a_l^{(0)}+\epsilon a_l^{(1)}+\epsilon^2 a_l^{(2)}.
\end{displaymath} (8)

Substituting this expansion in (7) we get in the zeroth order $ a_l^{(0)}(T)=a_l(0)
$, i.e. the zeroth order term is time independent. This corresponds to the fact that the interaction representation wave amplitudes are constant in the linear approximation. For simplicity, we will write $a^{(0)}_l(0)= a_l$, understanding that a quantity is taken at $T=0$ if its time argument is not mentioned explicitly. The first order is given by
$\displaystyle a^{(1)}_l (T) = -i \sum_{m,n=1}^\infty \left( V^l_{mn} a_m
a_n \D...
...l_{m+n}
+ 2
\bar{V}^m_{ln}a_m\bar{a}_n \bar\Delta^m_{ln}\delta^m_{l+n}
\right),$     (9)

where $ \Delta^l_{mn}=\int_0^T e^{i\omega^l_{mn}t}d t =
({e^{i\omega^l_{mn}T}-1})/{i \omega^l_{mn}}.
$ Here we have taken into account that $a^{(0)}_l(T)= a_l$ and $a^{(1)}_k (0)=0$. Iterating one more time we get


$\displaystyle a_l^{(2)} (T)$ $\textstyle =$ $\displaystyle \sum_{m,n, \mu, \nu}^\infty \left[ 2
V^l_{mn} \left( -V^m_{\mu \n...
...l \nu}_{n
\mu},\omega^l_{mn}]\delta^\mu_{m + \nu}\right) \delta^l_{m+n}
\right.$  
    $\displaystyle \left. + 2 \bar V^m_{ln}
\left(-V^m_{\mu \nu}\bar a_n a_\mu a_\nu...
...{n \nu l},-\omega^m_{l n}] \delta^\mu_{m +
\nu} \right) \delta^m_{l+ n} \right.$  
    $\displaystyle \left. + 2 \bar
V^m_{ln} \left( \bar V^n_{\mu \nu}a_m \bar a_\mu ...
...u l}_{\nu m},
-\omega^m_{ln}]\delta^\mu_{n + \nu}\right)\delta^m_{l+n}
\right],$  

where we used $a^{(2)}_k (0)=0$ and introduced $E(x,y)=\int_0^T \Delta(x-y)e^{i y t} d t .$


next up previous
Next: Evolution of the multi-mode Up: Joint statistics of amplitudes Previous: Definition of an essentially
Dr Yuri V Lvov 2007-01-17