
Boundary, spectral and evolution
problems
A quick classification of various mathematical problems encountered in the modelization
of physical phenomena is proposed in the present chapter. More precisely, the problems
considered in this chapter are those that can be reduced to the finding of the solution of a
partial differential equation (PDE). Indeed, for many physicists, to provide a model of a
phenomenon means to provide a PDE describing this phenomenon. They can be
boundary problems, spectral problems, evolution problems. General ideas about the
methods of exact and approximate solving of those PDE is also proposed\footnote{The
reader is supposed to have a good knowledge of the solving of ordinary differential
equations. A good reference on this subject is ).}. This chapter contains numerous
references to the "physical" part of this book which justify the interest given to those
mathematical problems.
In classical books about PDE, equations are usually classified into three categories:
hyperbolic, parabolic and elliptic equation. This classification is connected to the proof of
existence and unicity of the solutions rather than to the actual way of obtaining the
solution. We present here another classification connected to the way one obtains the
solutions: we distinguish mainly boundary problems and evolution problems.
Let us introduce boundary problems:
Problem: (Boundary problem) Find u such that:
1.
1. u satisfies the boundary conditions.
This class of problems can be solved by integral methods section chapmethint) and by
variational methods section chapmetvar). Let us introduce a second class of problems:
evolution problems. Initial conditions are usually implied by time variables. One knows
at time t
0
the function u(x,y,t )
0
and try to get the values of u(x,y,t) for t greater than t
0
.
This our second class of problem:
Problem: (Evolution problem) Find such that: