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Next: A Higher-Order Korteweg-de Vries Up: The Painlevé Property for Previous: The Modified KdV Equation

The Bousinesq Equation

The Bousinesq equation

\begin{displaymath}u_{tt}+{\partial^2\over\partial x^2}\left({u_{xx}\over 3}+u^2\right)
=0\eqno (4.1)\end{displaymath}

possesses the Painlevé property [1].

In general, it is found that

\begin{displaymath}u=\phi^{-2}\sum_{j=0}^{\infty} u_j\phi^j ,\eqno (4.2)\end{displaymath}

where the resonances occur at

\begin{displaymath}j=-1,4,5,6 .\eqno (4.3)\end{displaymath}

The compatability conditions at $j=4,5$, and 6 are satisfied identically. We will require that

\begin{displaymath}u_3=0\eqno (4.4)\end{displaymath}

and set

\begin{displaymath}u_4=u_5=u_6=0\eqno (4.5)\end{displaymath}

(implying $u_j=0\ge j\ge 3$). We find the associated Bäcklund transform

\begin{displaymath}u=2{\partial^2\over\partial x^2}\ln\phi+u_2 ,\eqno (4.6)\end{displaymath}

where $(u,u_2)$ satisfy (4.1), and

\begin{displaymath}\phi_t^2-\phi_{xx}^2+\textstyle{4\over 3}\phi_x\phi_{xxx}+2u_2\phi_x^2=0 ,
\eqno (4.7)\end{displaymath}


\begin{displaymath}\phi_{tt}+\textstyle{1\over 3}\phi_{xxxx}+2\phi_{xx} u_2=0 .\eqno (4.8)\end{displaymath}

Now, by eliminating $u_2$ in (4.7) and (4.8), it is found that

\begin{displaymath}{\partial\over\partial t}\left({\phi_t\over\phi_x}\right)+{1\...
...{1\over 3}
{\partial\over\partial x}\{\phi;x\}=0 ,\eqno (4.9)\end{displaymath}

where $\{\phi;x\}$ is the Schwarzian derivative.

As before, this equation is invariant under the Moebius group. We let

\begin{displaymath}\phi=v_1/v_2\eqno (4.10)\end{displaymath}

and find

\begin{displaymath}{\partial\over\partial t}\left({\psi_t\over\theta_x}\right)+{...
...eta_{xx}\over\theta_x}{v_{2x}\over v_2}\right)=0 ,\eqno (4.11)\end{displaymath}

where

\begin{displaymath}\theta_x=v_2v_{1x}-v_1v_{2x} ,\eqno (4.12)\end{displaymath}


\begin{displaymath}\psi_t=v_2v_{1t}-v_1v_{2t} ,\eqno (4.13)\end{displaymath}

and

\begin{displaymath}\{\theta;x\}={\partial\over\partial x}\left({\theta_{xx}\over...
...er 2}\left({\theta_{xx}\over\theta_x}\right)^2 .
\eqno (4.14)\end{displaymath}

To solve (4.11), first we let $(v_1,v_2)$ satisfy the following:

Second-order scattering problem:

\begin{displaymath}v_{xx}=av ,\eqno (4.15)\end{displaymath}


\begin{displaymath}v_t=bv_x+cv .\eqno (4.16)\end{displaymath}

Then,

\begin{displaymath}\theta_{xx}=0 ,\end{displaymath}


\begin{displaymath}\psi_t=b\theta_x ,\end{displaymath}

and from (4.11)

\begin{displaymath}b_t+bb_x=\textstyle{2\over 3}ax ,\eqno (4.17)\end{displaymath}

while by compatability of (4.15) and (4.16)

\begin{displaymath}\null \vcenter{\openup\jot
\ialign{\strut\hfil$\displaysty...
...{xx}=0 ,\cr
&a_t=c_{xx}+2ab_x+ba_x ,\cr\crcr}} \eqno (4.18)\end{displaymath}

or, collecting equations,

\begin{displaymath}\null \vcenter{\openup\jot
\ialign{\strut\hfil$\displaysty...
...
b_t&=-bb_x+\textstyle{2\over 3}a_x .\cr\crcr}} \eqno (4.19)\end{displaymath}

Unfortunately, it is not possible to introduce an arbitrary,spectral parameter

\begin{displaymath}a=u+\lambda\eqno (4.20)\end{displaymath}

into Eq. (4.15) without obtaining from (4.19) equations that will depend explicitly on that parameter. Therefore, we shall consider the following:

Third-order scattering problem:

\begin{displaymath}v_{xxx}=av_x+bv ,\eqno (4.21)\end{displaymath}


\begin{displaymath}v_t=cv_{xx}+dv_x+ev .\eqno (4.22)\end{displaymath}

Then,

\begin{displaymath}\psi_t=c\theta_{xx}+d\theta_x ,\eqno (4.23)\end{displaymath}

and substitution into (4.11) determines

\begin{displaymath}c^2=1 ,\qquad d=0\eqno (4.24)\end{displaymath}


\begin{displaymath}ce_x+\textstyle{2\over 3}a_x=0 .\eqno (4.25)\end{displaymath}

By the consistency condition for (4.21) and (4.22) we find

\begin{displaymath}\null \vcenter{\openup\jot
\ialign{\strut\hfil$\displaysty...
...xx} ,\cr
&b_t+ae_x=e_{xxx}+cb_{xx} .\cr\crcr}} \eqno (4.26)\end{displaymath}

Letting

\begin{displaymath}a=-\textstyle{3\over 2}ce ,\eqno (4.27)\end{displaymath}

we find

\begin{displaymath}ce_{tt}+{\partial^2\over\partial x^2}\left(e^2+c{e^{xx}\over 3}
\right)=0 ,\eqno (4.28)\end{displaymath}

where

\begin{displaymath}c^2=1 .\end{displaymath}

Let

\begin{displaymath}c=1 ;\end{displaymath}

then


truecm $e$ is a solution of the Bousinesq equation


truecm $a=-\textstyle{3\over 2}e ,$


truecm $b=\lambda-\textstyle{3\over 4}e_x^2-\textstyle{3\over 4}
\displaystyle{\int^x} e_t ,$


truecm $c=1 ,\qquad d=0 .$(4.29)


Equations (4.29) determine the Lax pair for the Bousinesq equation [7]. We note the appearance of the spectral parameter $\lambda$.


next up previous
Next: A Higher-Order Korteweg-de Vries Up: The Painlevé Property for Previous: The Modified KdV Equation
John Edward Weiss 2002-03-31