20.7 UNIQUENESS OF SOLUTIONS
Equation type Boundary Conditions
hyperbolic open Cauchy
parabolic open Dirichlet or Neumann
elliptic closed Dirichlet or Neumann
Table 20.1 The appropriate boundary conditions for different types of partial
differential equation.
conditionsuand∂u/∂ton the line segmentt=0,x=0toL, the solution is
specified in the shaded region.
As in the case of first-order PDEs, however, problems can arise. For example,
if for a hyperbolic equation the boundary curve intersects any characteristic
more than once then Cauchy conditions alongCcan overdetermine the problem,
resulting in there being no solution. In this case either the boundary curveC
must be altered, or the boundary conditions on the offending parts ofCmust be
relaxed to Dirichlet or Neumann conditions.
The general considerations involved in deciding which boundary conditions are
appropriate for a particular problem are complex, and we do not discuss them
any further here.§We merely note that whether the various types of boundary
condition are appropriate (in that they give a solution that is unique, sometimes
to within a constant, and is well defined) depends upon the type of second-order
equation under consideration and on whether the region of solution is bounded
by a closed or an open curve (or a surface if there are more than two independent
variables). Note that part of a closed boundary may be at infinity if conditions
are imposed onuor∂u/∂nthere.
It may be shown that the appropriate boundary-condition and equation-type
pairings are as given in table 20.1.
For example, Laplace’s equation∇^2 u= 0 is elliptic and thus requires either
Dirichlet or Neumann boundary conditions on a closed boundary which, as we
have already noted, may be at infinity if the behaviour ofuis specified there
(most oftenuor∂u/∂n→0 at infinity).
20.7 Uniqueness of solutions
Although we have merely stated the appropriate boundary types and conditions
for which, in the general case, a PDE has a unique, well-defined solution, some-
times to within an additive constant, it is often important to be able to prove
that a unique solution is obtained.
§For a discussion the reader is referred, for example, to P. M. Morse and H. Feshbach,Methods of
Theoretical Physics, Part I(New York: McGraw-Hill, 1953), chap. 6.