
CARTESIAN
SOLUTIONS
425
out, however, all solutions can
be
written as a linear sum (of potentially infinite
number of terms) of these separable solutions.
You
will
see
examples of this as the
chapter progresses. Using
this
form
for
@(x,
y,
z),
Laplace’s equation becomes
(11.4)
Each of the three
terms
on the
LHS
of
Equation 11.4 is a function of only one
of the independent variables.
This
means that,
for
example,
the
sum
of
the last two
terms
(1
1.5)
cannot depend
on
x.
A
quick look back at Equation
1
1.4 shows that this implies the
first term, itself, also cannot be a function of
x.
It obviously
is
not a function
of
y
or
z
either,
so
it must be equal to a constant:
Similar arguments can be made to isolate the other terms:
(11.6)
(11.7)
(11.8)
The
three
quantities
c,,
cy,
and
cz
are called separation constants. Notice that they
are not completely independent of one another, because Laplace’s equation requires
c,
+
cy
+
c,
=
0.
(11.9)
Consequently, only two
can
be chosen arbitrarily.
11.1.1
Each
of
the three separated equations (Equations 11.6-1 1.8) is the same linear,
second-order differential equation. The solution to Equation
1
1.6,
for a particular,
nonzero value
of
c,,
is
simply
Solutions
of
the Separated
Equations
X(x)
=
x+e+@
+
x-e-fi,
c,
#
0,
(11.10)
where
X+
and
X-
are arbitrary amplitudes, which are determined only when we apply
the boundary conditions. When
this
general solution is combined with
Y
(y)
and
Z(z),
these constants combine with the corresponding
Yt
and
Zt
constants to
form
other
constants.
For
this reason, we will ignore these amplitude constants until the final