Further Properties of Laplace Transforms

Three properties turn a short table into a large one. Exponential scaling says multiplying f ( t ) by e a t shifts the transform to F ( s a ) . Time scaling says stretching time compresses frequency. And differentiating the transform corresponds to multiplying by t . Together they generate almost every transform needed in practice from the handful computed in Section 7.1.

Quick Reference

Property Statement Valid for
Linearity { a f + b g } = a F ( s ) + b G ( s ) both transforms exist
Exponential scaling { e a t f ( t ) } = F ( s a ) s > k + a
Time scaling { f ( a t ) } = 1 a F ( s a ) , a > 0 s > k a
Derivative of transform \mathscr{L}\left\{t\,f(t)\right\} = -F'(s) s > k
General form { t n f ( t ) } = ( 1 ) n d n d s n F ( s ) n = 1 , 2 , 3 ,

Transforms these generate:

f ( t ) F ( s )
t n e a t n ! ( s a ) n + 1
e a t sin k t k ( s a ) 2 + k 2
e a t cos k t s a ( s a ) 2 + k 2
t sin k t 2 k s ( s 2 + k 2 ) 2
t cos k t s 2 k 2 ( s 2 + k 2 ) 2

Exponential Scaling

In Section 7.1 we learned that is a linear operator. We now study some further properties.

Exponential Scaling (also called the first shifting theorem). If { f ( t ) } = F ( s ) exists for s > k 0 and a is a constant, then

{ e a t f ( t ) } = F ( s a )

for s a > k , that is, for s > k + a .

Proof\begin{aligned} \mathscr{L}\left\{e^{at}f(t)\right\} &= \int_0^{\infty}e^{-st}e^{at}f(t)\,dt \\ &= \int_0^{\infty}e^{-(s-a)t}f(t)\,dt \\ &= F(s-a) . \end{aligned}

The last step is just the definition of F , read with s a in place of s . Nothing is required beyond combining the two exponentials.

In words: multiplying by e a t in the t domain translates the transform by a in the s domain. This is the single most useful property in the chapter. Read backwards, it says that whenever s appears only in the combination s a , an exponential factor e a t is present in f .

Find { t 2 e 4 t } .

Solution

We know { t n } = n ! s n + 1 for s > 0 . With n = 2 ,

{ t 2 } = 2 s 3 .

Applying the theorem with a = 4 , replace s by s 4 :

{ t 2 e 4 t } = 2 ( s 4 ) 3

valid for s 4 > 0 , that is, s > 4 .

Find { e t sin 3 t } .

Solution

Since { sin k t } = k s 2 + k 2 for s > 0 , taking k = 3 gives

{ sin 3 t } = 3 s 2 + 9 .

Applying the theorem with a = 1 , replace s by s ( 1 ) = s + 1 :

{ e t sin 3 t } = 3 ( s + 1 ) 2 + 9

valid for s + 1 > 0 , that is, s > 1 .

Note that only the s in the transform is replaced; the constant k = 3 in the numerator is untouched. Replacing s everywhere, including inside k 2 , is a common slip.

Time Scaling

Time Scaling. If { f ( t ) } = F ( s ) exists for s > k 0 and a is a positive constant, then

{ f ( a t ) } = 1 a F ( s a )

for s / a > k , that is, s > k a .

Proof

Substitute τ = a t , so t = τ / a and d t = d τ / a :

{ f ( a t ) } = 0 e s t f ( a t ) d t = 0 e s τ / a f ( τ ) d τ a = 1 a 0 e ( s / a ) τ f ( τ ) d τ = 1 a F ( s a ) .

The requirement a > 0 keeps the limits of integration in order.

The theorem makes physical sense: if time is scaled by a , frequency is scaled by 1 / a . Playing a recording twice as fast doubles every frequency, and the extra factor 1 / a out front conserves the total.

Given { sin t } = 1 s 2 + 1 and { cos t } = s s 2 + 1 , find { sin k t } and { cos k t } .

Solution

Applying the theorem with a = k > 0 ,

\begin{aligned} \mathscr{L}\left\{\sin kt\right\} &= \frac{1}{k}\cdot\frac{1}{(s/k)^{2}+1} \\ &= \frac{1}{k}\cdot\frac{k^{2}}{s^{2}+k^{2}} \\ &= \frac{k}{s^{2}+k^{2}} \end{aligned}

where the middle step multiplied numerator and denominator by k 2 .

Similarly,

\begin{aligned} \mathscr{L}\left\{\cos kt\right\} &= \frac{1}{k}\cdot\frac{s/k}{(s/k)^{2}+1} \\ &= \frac{1}{k}\cdot\frac{sk}{s^{2}+k^{2}} \\ &= \frac{s}{s^{2}+k^{2}} \end{aligned}

Both agree with the direct computations of Section 7.1, obtained here with far less work.

Derivatives of a Transform

Derivatives of a Transform. If { f ( t ) } = F ( s ) , then

\mathscr{L}\left\{t\,f(t)\right\} = -F'(s)

and in general

{ t n f ( t ) } = ( 1 ) n d n d s n F ( s ) ( n = 1 , 2 , 3 , ) .
Proof

Differentiate both sides of F ( s ) = 0 e s t f ( t ) d t with respect to s , moving the derivative inside the integral:

\begin{aligned} \frac{d}{ds}F(s) &= \frac{d}{ds}\int_0^{\infty}e^{-st}f(t)\,dt \\ &= \int_0^{\infty}\frac{\partial}{\partial s}\left[e^{-st}f(t)\right]dt \\ &= \int_0^{\infty}(-t)e^{-st}f(t)\,dt \\ &= -\int_0^{\infty}e^{-st}\,t\,f(t)\,dt \\ &= -\mathscr{L}\left\{t\,f(t)\right\} \end{aligned}

The interchange of differentiation and integration is justified when f satisfies the conditions of the existence theorem.

Applying the result to t f ( t ) in place of f ,

\begin{aligned} \mathscr{L}\left\{t^{2}f(t)\right\} &= \mathscr{L}\left\{t\cdot t f(t)\right\} \\ &= -\frac{d}{ds}\mathscr{L}\left\{t f(t)\right\} \\ &= -\frac{d}{ds}\left(-\frac{d}{ds}\mathscr{L}\left\{f(t)\right\}\right) \\ &= \frac{d^{2}}{ds^{2}}F(s) . \end{aligned}

Repeating gives

{ t n f ( t ) } = ( 1 ) n d n d s n F ( s ) ,

with the sign alternating because each application contributes one factor of 1 .

Note the pleasing symmetry with Section 7.5: differentiating in t corresponds (roughly) to multiplying by s , and differentiating in s corresponds to multiplying by t . The two variables trade roles.

Find { t sin k t } .

Solution

Since { sin k t } = k s 2 + k 2 , the theorem gives

\begin{aligned} \mathscr{L}\left\{t\sin kt\right\} &= -\frac{d}{ds}\left(\frac{k}{s^{2}+k^{2}}\right) \\ &= -\frac{\dfrac{d}{ds}(k)\cdot\left(s^{2}+k^{2}\right) - k\cdot\dfrac{d}{ds}\left(s^{2}+k^{2}\right)}{\left(s^{2}+k^{2}\right)^{2}} \\ &= -\frac{0\cdot\left(s^{2}+k^{2}\right) - k(2s)}{\left(s^{2}+k^{2}\right)^{2}} \\ &= \frac{2ks}{\left(s^{2}+k^{2}\right)^{2}} \end{aligned}

Remember that k is a constant while s is the variable, so d k d s = 0 and d d s ( s 2 + k 2 ) = 2 s .

Find { t 2 e 3 t } by two different routes.

Solution

Method (a): differentiate the transform. Start from { e a t } = 1 s a with a = 3 :

{ e 3 t } = 1 s + 3 .

Then

\begin{aligned} \mathscr{L}\left\{t^{2}e^{-3t}\right\} &= \frac{d^{2}}{ds^{2}}\left[(s+3)^{-1}\right] \\ &= \frac{d}{ds}\left[-(s+3)^{-2}\right] \\ &= 2(s+3)^{-3} = \frac{2}{(s+3)^{3}} \end{aligned}

Method (b): use exponential scaling. Start from { t n } = n ! s n + 1 with n = 2 :

{ t 2 } = 2 s 3 .

By the exponential scaling theorem, replace s by s + 3 :

{ t 2 e 3 t } = 2 s 3 | s s + 3 = 2 ( s + 3 ) 3 .

Method (b) is much shorter, and it generalizes at once to { t n e a t } = n ! ( s a ) n + 1 , a formula worth memorizing.

Find { t cos k t } .

Solution

Starting from { cos k t } = s s 2 + k 2 and applying the quotient rule,

\begin{aligned} \mathscr{L}\left\{t\cos kt\right\} &= -\frac{d}{ds}\left(\frac{s}{s^{2}+k^{2}}\right) \\ &= -\frac{1\cdot\left(s^{2}+k^{2}\right) - s(2s)}{\left(s^{2}+k^{2}\right)^{2}} \\ &= -\frac{k^{2}-s^{2}}{\left(s^{2}+k^{2}\right)^{2}} = \frac{s^{2}-k^{2}}{\left(s^{2}+k^{2}\right)^{2}} \end{aligned}

This transform appears constantly in resonance problems, where the factor t is what the Modification Rule of Section 4.3 predicted.

Exercises

Find { e 2 t cos 5 t } .

Solution

Since { cos 5 t } = s s 2 + 25 , exponential scaling with a = 2 gives

{ e 2 t cos 5 t } = s 2 ( s 2 ) 2 + 25 ,

valid for s > 2 . Note that the numerator becomes s 2 , not s : every s in the transform is replaced.

Find { t 3 e 2 t } .

Solution

Since { t 3 } = 6 s 4 , replacing s by s + 2 gives

{ t 3 e 2 t } = 6 ( s + 2 ) 4 .

Find { t 2 sin t } .

Solution

Start from F ( s ) = 1 s 2 + 1 and differentiate twice, using n = 2 so the sign is ( 1 ) 2 = + 1 .

First derivative: F'(s) = -\dfrac{2s}{\left(s^{2}+1\right)^{2}}.

Second derivative, by the quotient rule:

F''(s) = -\frac{2\left(s^{2}+1\right)^{2} - 2s\cdot 2\left(s^{2}+1\right)(2s)}{\left(s^{2}+1\right)^{4}} = -\frac{2\left(s^{2}+1\right) - 8s^{2}}{\left(s^{2}+1\right)^{3}} = \frac{6s^{2}-2}{\left(s^{2}+1\right)^{3}} .

Therefore

{ t 2 sin t } = 6 s 2 2 ( s 2 + 1 ) 3 .

Given that { f ( t ) } = 1 s 2 + 1 , find { f ( 3 t ) } without identifying f .

Solution

By time scaling with a = 3 ,

{ f ( 3 t ) } = 1 3 1 ( s / 3 ) 2 + 1 = 1 3 9 s 2 + 9 = 3 s 2 + 9 .

As a check, f ( t ) = sin t so f ( 3 t ) = sin 3 t , whose transform is indeed 3 s 2 + 9 .

Frequently Asked Questions

What is the exponential scaling theorem?

It states that { e a t f ( t ) } = F ( s a ) : multiplying by an exponential in t shifts the transform in s . It is often called the first shifting theorem, to distinguish it from the time-shifting theorem of Section 7.6.


How do I apply the shift correctly?

Compute F ( s ) for the function without the exponential, then substitute s a for every occurrence of s . For e t sin 3 t : first get 3 s 2 + 9 , then replace s by s + 1 to get 3 ( s + 1 ) 2 + 9 . The constant 3 in the numerator is not an s , so it stays.


Why does { t f ( t ) } carry a minus sign?

Because differentiating e s t with respect to s brings down a factor of t . Each further differentiation brings down another, which is why the general formula carries ( 1 ) n .


Which property should I use for t n e a t ?

Exponential scaling, applied to { t n } = n ! s n + 1 , gives n ! ( s a ) n + 1 in one step. Differentiating the transform n times reaches the same answer with far more algebra. When two routes exist, the shifting theorem is almost always the shorter one.


Why must a be positive in the time-scaling theorem?

Because the substitution τ = a t must preserve the orientation of the interval [ 0 , ) . A negative a would map it to ( , 0 ] , which lies outside the range the unilateral transform can see.