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Sine-Gordon Solitons

Author of Web page:
Guillermo Avendaño Franco

Léalo en Español

From field theory the wave equation for mesons is
\begin{displaymath}
\nabla^{2}u(x,t)-\frac{\partial^2 u(x,t)}{\partial t^2}=m^2 u(x,t)+g^2
u^3(x,t),
\end{displaymath} (1)

the right hand side is the addition of the two first terms of the sin series

\begin{displaymath}
{\rm sen}(x)=\sum^{\infty}_{n=0}(-1)^n\frac{x^{2n+1}}{(2n+1)!}
\end{displaymath}

taking$m=1$ and$g=\sqrt{-1/6}$, then the bidimensional equation takes the form
\begin{displaymath}
\frac{\partial^2 u}{\partial x^2}+\frac{\partial^2 u}{\partial
y^2}-\frac{\partial^2 u}{\partial t^2}={\rm sen}(u).
\end{displaymath} (2)



The non-linearity of Sine-Gordon Eq. (1) makes difficult to obtain an analytic solution. To find a numeric solution lets start limiting the working space:

\begin{displaymath}
-x_0<x<x_0 \ \ -y_0<y<y_0 \ \ t\geq 0,
\end{displaymath} (3)

with $x_0=y_0=7$, additionally the spatial derivate is taken zero on the borders.
\begin{displaymath}
\frac{\partial u}{\partial x}(-x_0,y ,t)=\frac{\partial u}{\partial x}(x_0,y ,t)=0
\end{displaymath} (4)



\begin{displaymath}
\frac{\partial u}{\partial y}(x,-y_0 ,t)=\frac{\partial
u}{\partial y}(x,y_0,t)=0.
\end{displaymath} (5)

As initial condition the function: $u$ is selected, and its derivate at time$t=0$ :
\begin{displaymath}
u(x,y,t=0)=4 \tan^{-1}(e^{3-\sqrt{x^{2}+y^{2}}})
\end{displaymath} (6)


\begin{displaymath}
\frac{\partial u}{\partial x}(x,y ,t=0)=0.
\end{displaymath} (7)


Space and time are discretized as:

Continuous $\Rightarrow$ Discret
$(x,y,t)$ $\rightarrow$ $(m,l,n)$

\begin{displaymath}
x = m\, \Delta x,\ \ y = l\, \Delta y,\ \ t = n\, \Delta t,
\end{displaymath} (8)

with $\Delta x=\Delta y$
Time is expresed with a superscript:

\begin{displaymath}
u^{n}_{m,l}\equiv u(m\ \Delta x,l\ \Delta x,n\ \Delta t,).
\end{displaymath} (9)

the usual expansions for second derivatives :
$\displaystyle u_{m,l}^{n+1}\simeq$ $\textstyle -$ $\displaystyle u^{n-1}_{m,l}+2\left[1-2\left( \frac{\Delta t}{\Delta x}\right)^{2}\right]\ u^{n}_{m,l}$ (10)
  $\textstyle +$ $\displaystyle \left( \frac{\Delta t}{\Delta
x}\right)^{2}(u^{n}_{m+1,l}+u^{n}_{m-1,l}+u^{n}_{m,l+1}+u^{n}_{m,l-1})$ (11)
  $\textstyle -$ $\displaystyle \Delta t^{2} {\rm sen}\left[\frac{1}{4}(u^{n}_{m+1,l}+u^{n}_{m-1,l}+u^{n}_{m,l+1}+u^{n}_{m,l-1})\right],$ (12)

and to guarantee stability varibles$\Delta x$ and$\Delta t$ are related by:
\begin{displaymath}
\Delta x = \sqrt{2}\ \Delta t
\end{displaymath} (13)

To learn more about sine-Gordon equation see: Landau R.H. and Paez M.J., (1997) Computational Physics , John Wiley and Sons, New York.

An algorithm was written to create 3-D images and an animation using software such as ppmtogif and GIFmerge

GIFmerge can be download at
http://www.uni-jena.de/~nmh/gcms/dok/gifmerge/docu/

This animation shows the beginning of the soliton motion