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Laplace and Poisson Equations

The Laplace equation (in 2-D)

\begin{displaymath}\nabla^2 u = \frac{\partial^2 u}{\partial x^2} +
\frac{\partial^2 u}{\partial x^2} = 0
\end{displaymath} (7)

and the Poisson equation (in 2-D)

\begin{displaymath}\nabla^2 u = \frac{\partial^2 u}{\partial x^2} +
\frac{\partial^2 u}{\partial x^2} = S(x,y)
\end{displaymath} (8)

are encountered in the solution for potential functions, for instance in electrostatic and gravitational problems, and in describing the steady state reached in heat transmission problem. The function u(x,y) is a time independent field, i.e., a potential or a temperature profile function; S(x,y) represent a source term, i.e., a mass distribution, a charge distribution, or a heat source.

These equations are said to be of Elliptic type. No time dependence is involved here. A time independent solution for u(x,y) is sought after within a domain $\Omega$. In 2-D the domain could be a simple rectangle, $0 \le x \le 1$ and $0 \le y \le 1$, or could be of arbitrary shape.

The solution, or its derivative, is specified at the boundary of the domain, $\Gamma$. The possibilities are:

1.
Dirichlet Boundary conditions, in which the function is specified on the boundary of the domain

u(x,y) = f(x,y), (9)

2.
Newman boundary conditions, in which the normal derivative is specified,

\begin{displaymath}\frac{\partial u}{\partial n} = g(x,y),
\end{displaymath} (10)

3.
The Fourier case in which a mix of function values and normal derivatives is specified.


next up previous
Next: Numerical Solution Up: No Title Previous: Finite Difference Approach
Michel Vallieres
2001-05-11