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Solving linear differential equations using the
Laplace transform
The Laplace transform, the basics of which have been introduced in
the sections above, is an elegant way for fast and schematic
solving of linear differential equations with constant
coefficients. In the following the importance of this approach is
demonstrated. Instead of solving the differential equation with
the initial conditions directly in the original domain, the detour
via a mapping into the frequency domain is
taken, where only an algebraic equation has to be solved. Thus
solving differential equations is performed according to
Figure 2.2 in the following three steps:
- Transformation of the differential equation into the mapped
space,
- Solving the
algebraic
equation in the
mapped space,
- Back transformation of the solution into the original space.
Figure 2.2:
Schema for solving differential equations using the Laplace transformation
 |
Whereas the first two steps are trivial, the third step usually
demands more effort. The procedure will be demonstrated by the
following two examples.
Example 2.5.1
Consider the differential equation
with the initial conditions

.
Proceeding using the steps given above one has
- Step 1:
- Step 2:
- Step 3:
The complex function
must be decomposed into partial fractions
in order to use the tables
of correspondences. This gives
By means of the correspondences 6 and 7 of Table 2.1
it follows from the inverse Laplace transformation that the solution of the
given differential equation is
Example 2.5.2
Given the differential equation
 |
(2.30) |
where

and

are constants and the initial conditions

and

are known. Then
- Step 1:
- Step 2:
 |
(2.31) |
with the abbreviation
and |
|
- Step 3:
Case a): two single real zeros of the denominator:
This means
For both rational expressions
and
it follows
by partial fraction decomposition that
and |
|
The coefficients
and
can now be determined by
comparing coefficients or by applying Eq. (2.22):
for  |
|
Thus for Eq. (2.31) follows
and by applying the correspondence 6 from Table 2.1
the solution of the differential equation is
Case b): One double real zero of the denominator:
Here is
For the two rational expressions
and
of
Eq. (2.31) the partial fraction decomposition is
and  |
|
The coefficients
and
are determined by comparing
both sides or by evaluation of Eq. (2.25):
and
From these results one obtains the solution
in the mapped space. By applying the inverse Laplace
transformation the required solution of the differential equation
is
 |
(2.33) |
Case c): Two conjugate complex zeroes of the denominator:
Here
with |
|
Introducing the values of
and
and after
multiplication of this expression one obtains
Comparison with the denominator of the original relation,
Eq. (2.31), gives according to Eq. (2.28)
and  |
|
With these coefficients Eq. (2.31) is in the form
and from this one gets by applying the correspondences
15 and 16 of Table 2.1 to
the corresponding time function
or rearranged
 |
(2.34) |
Also from Eq. (2.31) of this example the importance of
the position of the zeros of
, the poles of
, on the
solution is clear. For all three cases the solution of the
differential equation according to Eqs. (2.32),
(2.33) and (2.34) is mainly influenced by
the position of the poles of
. These poles of
are -
as one can see from the two examples - only depend on the left
side of the corresponding differential equation, i.e. the
homogeneous part of it. As is generally known the solution of the
homogeneous differential equation describes the modes of the system, that is the behaviour,
which depends only on the initial conditions.
Therefore, consider for the general case only the homogeneous part
of an
th-order ordinary homogeneous linear differential
equation with constant coefficients that is
 |
(2.35) |
with all
initial conditions
for |
|
One obtains by Laplace transformation
and a form according to Eq. (2.31)
 |
(2.36) |
where
and
are polynomials in
and the initial
conditions are only in the numerator polynomial
. The poles
of
can be determined
directly from the solution of the equation
 |
(2.37) |
After factorisation of this equation one obtains
 |
(2.38) |
The poles
of
make it possible to perform a
partial fraction
decomposition of
, e.g. for the case of single poles
according to Eq. (2.20). For this case one obtains
following Eq. (2.21) the solution of the homogeneous
differential equation, Eq. (2.35), in the form
for  |
|
From this one can realise that the position of the poles
of
in the
plane
completely characterises the
modes or inherent behaviour of the system described
by Eq. (2.35). Thus one obtains for
(left-half
plane) a
decreasing and for
(right-half
plane) an increasing behaviour of
,
while for pairs of poles with
permanent oscillations occur. Therefore,
Eq. (2.37) or equivalently
Eq. (2.38), is called the
characteristic equation
and the poles
of
are often called
eigenvalues of the equation. Therefore
investigation of the characteristic equation provides the most
important information about the oscillating behaviour of a system.
Next: Laplace transform of the
Up: The Laplace transform
Previous: The inverse Laplace transform
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Christian Schmid 2005-05-09