A particular kind of integral transformation is known as the
Laplace transformation, denoted by
L. The definition of this operator is
The result—called the
Laplace transform of
f—will be a function of
p, so in general,
Example 1: Find the Laplace transform of the function
f(
x) =
x.
By definition,
Integrating by parts yields
Therefore, the function
F(
p) = 1/
p2 is the Laplace transform of the function
f(
x) =
x. [Technical note: The convergence of the improper integral here depends on
p being positive, since only then will (
x/p)
e−
px
and
e−
px
approach a finite limit (namely 0) as
x → ∞. Therefore, the Laplace transform of
f(
x) =
x is defined only for
p > 0.]
In general, it can be shown that for any nonnegative integer
n,
Like the operators
D and
I—indeed, like all operators—the Laplace transform operator
L acts on a function to produce another function. Furthermore, since
and
the Laplace transform operator
L is also linear.
[Technical note: Just as not all functions have derivatives or integrals, not all functions have Laplace transforms. For a function
f to have a Laplace transform, it is sufficient that
f(
x) be continuous (or at least piecewise continuous) for
x ≥ 0 and of
exponential order (which means that for some constants
c and λ, the inequality
holds for all
x). Any
bounded function (that is, any function
f that always satisfies |
f(
x)| ≤
M for some
M ≥ 0) is automatically of exponential order (just take
c =
M and λ = 0 in the defining inequality). Therefore, sin
kx and cos
kx each have a Laplace transform, since they are continuous and bounded functions. Furthermore, any function of the form
e
kx
, as well as any polynomial, is continuous and, although unbounded, is of exponential order and therefore has a Laplace transform. In short, most of the functions you are likely to encounter in practice will have Laplace transforms.]
Example 2: Find the Laplace transform of the function
f(
x) =
x3 – 4
x + 2.
Recall form the first statement following Example 1 that the Laplace transform of
f(
x) =
x
n
is
F(
p) =
n!/
p
n + 1
. Therefore, since the Laplace transform operator
L is linear,
Example 3: Determine the Laplace transform of
f(
x) =
e
kx
.
Apply the definition and perform the integration:
In order for this improper integral to converge, the coefficient (
p –
k) in the exponential must be positive (recall the technical note in Example 1). Thus, for
p >
k, the calculation yields
Example 4: Find the Laplace transform of
f(
x) = sin
kx.
By definition,
This integral is evaluated by performing integration by parts twice, as follows:
so
Therefore,
for
p > 0. By a similar calculation, it can be shown that
Example 5: Determine the Laplace transform of the function
pictured in Figure
1 :
This is an example of a
step function. It is not continuous, but it is
piecewise continuous, and since it is bounded, it is certainly of exponential order. Therefore, it has a Laplace transform.
Table
1 assembles the Laplace transforms of a few of the most frequently encountered functions, as well as some of the important properties of the Laplace transform operator
L.
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TABLE 1
|
Laplace Transforms
|
|
f(
x)
|
|
F(
p)
|
|
1
|
|
|
|
x
n
|
|
|
|
e
kx
|
|
|
|
sin
kx
|
|
|
|
cos
kx
|
|
|
|
Linearity:
|
|
|
|
Shifting formula:
|
|
|
|
Laplace transform of derivatives:
|
|
|
|
Example 6: Use Table
1 to find the Laplace transform of
f(
x) = sin2
x.
Invoking the trigonometric identity
linearity of
L implies
Example 7: Use Table
1 to find the Laplace transform of
g(
x)
x3
e5x.
The presence of the factor
e5x suggests using the shifting formula with
k =5. Since
the shifting formula says that the Laplace transform of
f(
x)
e5x =
x3
e
5x
is equal to
F(
P – 5). In other words, the Laplace transform of
x3
e5x is equal to the Laplace transform of
x3 with the argument
p
shifted to
p – 5:
Example 8: Use Table
1 to find Laplace transform of
f(
x) =
e−2x sin
x – 3.
First, since
L [sin
x] = 1/(
p2 + 1), the shifting formula (with
k = −2) says
Now, because
L[3] = 3 ·
L[1] = 3/
p, linearity implies
Example 9: Use Table
1 to find a continuous function whose Laplace transform is
F(
p) = 12/
p5.
This example introduces the idea of the
inverse Laplace transform operator,,
L−1. The operator
L−1 will “un-do” the action of
L. Symbolically,
If you think of the operator
L as changing
f(
x) into
F(
p), then the operator
L−1 just changes
F(
P) back into
f(
x). Like
L, the inverse operator
L−1 is linear.
More formally, the result of applying
L−1 a function
F(
p) is to recover the continuous function
f(
x) whose Laplace transform is the given
F(
p). [This situation should remind remind you of the operators
D and
I (which are, basically, inverses of one another). Each will un-do the action of the other in the sense that if, say,
I changes
f(
x) into
F(
x), then
D will change
F(
x) back into
f(
x). In other words,
D =
I−1, so if you apply
I and then
D, you're back where you started.]
Using Table
1 (reading it from to left),
Example 10: Find the continuous function whose Laplace transform is
F(
p) = 1/(
p2 – 1).
By partial fraction decomposition,
Therefore, by linearity of
L−1,
Example 11: Determine
First, note that
p has been shifted to
p + 2 =
p – (-2). Therefore, since
the shifting formula (with
k = −2) implies
Example 12: Evaluate
Although
p2 – 6
p + 25 cannot be factored over the integers, it can be expressed as the sum of two squares:
Therefore,