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AUTHOR
-
Pierre SPITERI
: Doctor of Mathematical Sciences - Professor at the École nationale supérieure d'électronique, d'électrotechnique, d'informatique, d'hydraulique et de télécommunication in Toulouse, France
INTRODUCTION
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, we
discussed the numerical solution of stationary partial differential
equation problems using the finite difference method. This method
can be extended to the solution of evolution problems. We will study
two types of problem: firstly, first-order evolution problems in time,
also known as parabolic problems
and, secondly, second-order evolution problems in time, also known
as hyperbolic problems
. The equations
involved in these problems consist partly of a combination of partial
derivatives with respect to the temporal variable, the numerical treatment
of which we shall describe in detail, and partly of a combination
of partial derivatives with respect to the spatial variable; the latter
part was dealt with in detail in the article
, the problem can be posed in a domain Ω, one-dimensional,
two-dimensional or three-dimensional; to simplify the presentation
we'll consider the domain to be the segment [0, 1], the two- and three-dimensional
case presenting no major difficulties.
Note :
The study of the finite-difference method for solving partial
differential equations is divided into three sections:
Finite difference
method for stationary PDEs ;
— [AF 501] Finite difference method for evolution PDEs ;
Numerical algorithms
for solving large systems.
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Finite-difference method for evolution PDEs