Mathematics for Electrical Science and Physical Science 1. Module 3, laplace transforms, inverse transforms and solving initial value problems.

GYMAT101 · 12 pages · Your place is saved in this browser

Contents · Laplace Transforms and Their Applications
Text size18

Laplace Transforms and Their Applications

Master the theory and application of the Laplace transform to evaluate transforms of elementary functions, invert rational frequency-domain functions, and solve initial value ordinary differential equations.

Before you start: Differential calculus including derivatives of polynomial, exponential, and trigonometric functions; Integral calculus including integration by parts and definite integration; Algebraic techniques including partial fraction decomposition and completing the square.

Your path through this module

  1. Definition and Elementary Laplace Transforms: An improper integral containing an exponential kernel transforms continuous time-domain functions into algebraic expressions in a new variable.
  2. First Shifting Theorem and Inverse Transforms: Multiplying by an exponential in the time domain corresponds directly to a simple horizontal shift in the s-domain.
  3. Transforms of Derivatives and ODE Solutions: Laplace transforms convert calculus operations into algebra by absorbing initial boundary conditions directly into the transform.
  4. The Convolution Integral and Inverse Products: The inverse transform of a product of two frequency-domain functions is the convolution integral of their respective time-domain originals.
  5. Discontinuous and Impulse Functions: Step and delta distributions allow piecewise and instantaneous inputs to be represented concisely and transformed into exponential s-domain terms.
  6. Computing Forward Transforms and Trigonometric Identities: Nonlinear time functions like products or powers of sinusoids must first be linearized using trigonometric identities before applying Laplace transforms.
  7. Inverse Transforms by Completing the Square: Completing the square exposes an internal s-shift, allowing quadratic denominators to be inverted into exponentially damped oscillatory functions.
  8. Inverse Transforms via Partial Fractions: Complex multi-pole rational functions decompose into a sum of simple first-order and power poles that each map directly to standard inverse formulas.
  9. Solving Initial Value Problems via Laplace Transforms: Differential equations are solved entirely within the algebraic s-domain, automatically packaging the initial state into the algebraic solution.
  10. Evaluating Inverse Transforms with the Convolution Theorem: Factoring a complicated transform into two simpler transforms converts an algebraic inversion problem into a single definite time integral.
  11. Transforming Delayed Step and Impulse Functions: Delayed activation and sudden spikes produce simple exponential phase factors e^(-as) in the frequency domain.

Definition and Elementary Laplace Transforms

In standard calculus, you learned how differentiation and integration act on functions of time, tt. The Laplace transform gives you a completely new perspective: it maps continuous functions of time into algebraic expressions of a new frequency variable, ss, allowing you to replace difficult calculus operations with simple algebra.

Think of a glass prism breaking a single beam of light into its component colors. The Laplace transform acts like a mathematical prism, breaking a continuous time signal into a spectrum of exponential building blocks. Each value of ss gauges how strongly a specific exponential mode is present in your original signal.

We define the unilateral Laplace transform of a function f(t)f(t), written as L{f(t)}\mathcal{L}\{f(t)\} or F(s)F(s), through an improper integral evaluated over positive time:

F(s)=∫0∞f(t)e−st dtF(s) = \int_{0}^{\infty} f(t)e^{-st} \, dt

The factor e−ste^{-st} is the kernel of the transform. Because ss is chosen to have a sufficiently large real part, e−ste^{-st} decays rapidly toward zero as tt grows, forcing the area under the curve to stay finite even for functions that grow over time.

Because integration is a linear operation, the Laplace transform inherits the linearity property. For any constants aa and bb, and functions f(t)f(t) and g(t)g(t):

L{af(t)+bg(t)}=aF(s)+bG(s)\mathcal{L}\{a f(t) + b g(t)\} = a F(s) + b G(s)

By evaluating the integral for basic building blocks, we obtain a standard catalog of elementary transforms valid for s>0s > 0 (or s>as > a):

f(t)f(t)F(s)=L{f(t)}F(s) = \mathcal{L}\{f(t)\}
11 (constant)1s\frac{1}{s}
tnt^n (nn is a positive integer)n!sn+1\frac{n!}{s^{n+1}}
eate^{at}1s−a\frac{1}{s - a}
cos⁡(ωt)\cos(\omega t)ss2+ω2\frac{s}{s^2 + \omega^2}
sin⁡(ωt)\sin(\omega t)ωs2+ω2\frac{\omega}{s^2 + \omega^2}
cosh⁡(at)\cosh(at)ss2−a2\frac{s}{s^2 - a^2}
sinh⁡(at)\sinh(at)as2−a2\frac{a}{s^2 - a^2}

Worked example

Find the Laplace transform of f(t)=4t3−5sin⁡(3t)+2e−4tf(t) = 4t^3 - 5\sin(3t) + 2e^{-4t}.

  1. Apply linearity to separate the expression into individual standard forms:
    L{f(t)}=4L{t3}−5L{sin⁡(3t)}+2L{e−4t}\mathcal{L}\{f(t)\} = 4\mathcal{L}\{t^3\} - 5\mathcal{L}\{\sin(3t)\} + 2\mathcal{L}\{e^{-4t}\}.
  2. Transform the power term t3t^3 using the rule tn→n!sn+1t^n \to \frac{n!}{s^{n+1}} with n=3n=3:
    L{t3}=3!s4=6s4\mathcal{L}\{t^3\} = \frac{3!}{s^4} = \frac{6}{s^4}.
  3. Transform the sine term sin⁡(3t)\sin(3t) using the rule sin⁡(ωt)→ωs2+ω2\sin(\omega t) \to \frac{\omega}{s^2 + \omega^2} with ω=3\omega=3:
    L{sin⁡(3t)}=3s2+9\mathcal{L}\{\sin(3t)\} = \frac{3}{s^2 + 9}.
  4. Transform the exponential term e−4te^{-4t} using eat→1s−ae^{at} \to \frac{1}{s-a} with a=−4a=-4:
    L{e−4t}=1s−(−4)=1s+4\mathcal{L}\{e^{-4t}\} = \frac{1}{s - (-4)} = \frac{1}{s + 4}.
  5. Combine the scaled components into a single ss-domain expression:
    F(s)=4(6s4)−5(3s2+9)+2(1s+4)=24s4−15s2+9+2s+4F(s) = 4\left(\frac{6}{s^4}\right) - 5\left(\frac{3}{s^2 + 9}\right) + 2\left(\frac{1}{s + 4}\right) = \frac{24}{s^4} - \frac{15}{s^2 + 9} + \frac{2}{s + 4}.

Remember

  • The unilateral transform integrates from t=0t = 0 to ∞\infty, weighted by the decaying kernel e−ste^{-st}.
  • Linearity permits term-by-term transformation of linear combinations.
  • Memorize the core transforms for 11, tnt^n, eate^{at}, cos⁡(ωt)\cos(\omega t), and sin⁡(ωt)\sin(\omega t) to rapidly build solutions.

First Shifting Theorem and Inverse Transforms

You already know how to transform basic signals like sine waves and powers of time into the ss-domain. Now we will learn how to handle signals that fade away over time, and how to translate ss-domain answers back into real time.

Think of plucking a guitar string: the sound does not ring forever, because friction makes the vibration die out exponentially. In math, we model this fading by multiplying a regular time function f(t)f(t) by an exponential factor eate^{at}. Because the Laplace integral already uses e−ste^{-st} as its kernel, multiplying by eate^{at} simply combines the exponents into e−(s−a)te^{-(s-a)t}. This gives us the first shifting theorem: if L{f(t)}=F(s)\mathcal{L}\{f(t)\} = F(s), then L{eatf(t)}=F(s−a)\mathcal{L}\{e^{at}f(t)\} = F(s - a). In plain words, multiplying by eate^{at} in time shifts every ss in the transform to s−as - a. If you draw a graph of F(s)F(s) against ss, this rule simply slides the whole curve horizontally by aa units.

Transforming a problem into the ss-domain is only half the job; at the end, we need a time function again. The inverse Laplace transform, written as L−1{F(s)}=f(t)\mathcal{L}^{-1}\{F(s)\} = f(t), is the operation that reverses the transform. It asks: what time signal f(t)f(t) produces this F(s)F(s)? Because the forward integral is linear, the inverse operator is also linear, meaning we can pull out constant multipliers and invert sums term by term.

Instead of computing a new integral to go backward, we read our basic transform table in reverse.

ss-domain F(s)F(s)Time-domain f(t)=L−1{F(s)}f(t) = \mathcal{L}^{-1}\{F(s)\}
n!sn+1\frac{n!}{s^{n+1}}tnt^n
ωs2+ω2\frac{\omega}{s^2 + \omega^2}sin⁡(ωt)\sin(\omega t)
s−a(s−a)2+ω2\frac{s - a}{(s - a)^2 + \omega^2}eatcos⁡(ωt)e^{at}\cos(\omega t)

Worked example

Find the inverse Laplace transform of F(s)=6(s+2)2+9F(s) = \frac{6}{(s + 2)^2 + 9}.

  1. Spot the shift: Notice that ss only appears inside the group (s+2)(s + 2), which matches s−as - a with a=−2a = -2. By the first shifting theorem, we can factor out the shift as e−2te^{-2t} in time and replace (s+2)(s + 2) with ss: L−1{6(s+2)2+9}=e−2tL−1{6s2+9}\mathcal{L}^{-1}\left\{\frac{6}{(s + 2)^2 + 9}\right\} = e^{-2t} \mathcal{L}^{-1}\left\{\frac{6}{s^2 + 9}\right\}.
  2. Match the base form: The remaining fraction has s2+32s^2 + 3^2 in the bottom, which matches the sine transform with ω=3\omega = 3.
  3. Adjust the constant using linearity: A sine transform needs ω=3\omega = 3 on top, so we rewrite 66 as 2×32 \times 3 and pull the 22 out front: 2e−2tL−1{3s2+32}=2e−2tsin⁡(3t)2e^{-2t} \mathcal{L}^{-1}\left\{\frac{3}{s^2 + 3^2}\right\} = 2e^{-2t}\sin(3t).

Remember

  • Multiplying by eate^{at} in time replaces every ss with s−as - a in the ss-domain.
  • To invert a shifted function, replace (s−a)(s - a) with ss, invert the simpler fraction, and multiply the result by eate^{at}.
  • The inverse transform is linear: split sums apart and factor constants out to match standard table forms.

Transforms of Derivatives and ODE Solutions

Now that you can move functions back and forth between the tt-domain and the ss-domain, we can see what the Laplace transform does to derivatives. This lets us turn differential equations into simple algebra problems.

Imagine tracking a moving car. To predict its future position, you need to know how fast it is moving and exactly where it started. An initial value problem is a differential equation paired with initial conditions, which are the known values of the function and its derivatives at time t=0t = 0. Usually, you solve the equation first and plug in these starting values at the very end. The Laplace transform is powerful because it absorbs those starting values right at the beginning.

When we apply the integral definition of the Laplace transform to a derivative y′(t)y'(t) and use integration by parts, the boundary at t=0t = 0 brings the starting value y(0)y(0) directly into the equation. If L{y(t)}=Y(s)\mathcal{L}\{y(t)\} = Y(s), the rule for the first derivative is L{y′(t)}=sY(s)−y(0)\mathcal{L}\{y'(t)\} = sY(s) - y(0). In plain words, taking a derivative in time becomes multiplying by ss in the frequency domain, minus the starting value. Applying this rule a second time gives the transform of the second derivative:

Time DomainFrequency Domain (ss-domain)
y(t)y(t)Y(s)Y(s)
y′(t)y'(t)sY(s)−y(0)sY(s) - y(0)
y′′(t)y''(t)s2Y(s)−sy(0)−y′(0)s^2Y(s) - sy(0) - y'(0)

To picture the complete solution pipeline, draw a square with four corners. Label the top-left corner "ODE in tt" and the top-right "ODE solution y(t)y(t)". Label the bottom-left "Algebraic equation in ss" and the bottom-right "Y(s)Y(s)". Instead of crossing the hard top path using calculus, you go down to the ss-domain using the derivative rules, walk across the bottom by algebraically isolating Y(s)Y(s), and climb back up to y(t)y(t) using the inverse transform.

Worked example

Solve the initial value problem y′(t)+2y(t)=0y'(t) + 2y(t) = 0, given the initial condition y(0)=3y(0) = 3.

  1. Transform the equation to turn calculus into algebra. Take the Laplace transform of each term using the first derivative rule:

    [sY(s)−y(0)]+2Y(s)=0[sY(s) - y(0)] + 2Y(s) = 0
  2. Insert the initial condition to include the starting state. Substitute y(0)=3y(0) = 3 into the brackets:

    sY(s)−3+2Y(s)=0sY(s) - 3 + 2Y(s) = 0
  3. Isolate Y(s)Y(s) to solve the problem in the ss-domain. Factor out Y(s)Y(s) and divide by (s+2)(s + 2):

    Y(s)(s+2)=3  ⟹  Y(s)=3s+2Y(s)(s + 2) = 3 \implies Y(s) = \frac{3}{s + 2}
  4. Invert to return to the time domain. Recognize the elementary form 1s−a\frac{1}{s - a} with a=−2a = -2 and apply the inverse transform:

    y(t)=L−1{3s+2}=3e−2ty(t) = \mathcal{L}^{-1}\left\{\frac{3}{s + 2}\right\} = 3e^{-2t}

Remember

  • Differentiation in the tt-domain turns into multiplication by ss in the ss-domain, minus the initial conditions.
  • Memorize the two core rules: L{y′}=sY(s)−y(0)\mathcal{L}\{y'\} = sY(s) - y(0) and L{y′′}=s2Y(s)−sy(0)−y′(0)\mathcal{L}\{y''\} = s^2Y(s) - sy(0) - y'(0).
  • Follow the three-step pipeline: transform the equation, solve algebraically for Y(s)Y(s), and invert to find y(t)y(t).

The Convolution Integral and Inverse Products

In the previous lesson, you solved differential equations by inverting rational expressions in the ss-domain. When a transform is a product of two simple terms that are hard to pull apart algebraically, this lesson gives you an integral tool to invert them directly.

Imagine striking a bell repeatedly with a hammer. The sound you hear right now is the sum of the fresh strike and the fading echoes of all earlier strikes. In engineering, we combine a current input with the fading memory of past inputs using an operation called convolution, written as (f∗g)(t)(f * g)(t). It takes two time-domain functions, f(t)f(t) and g(t)g(t), and blends them over the interval from 00 to tt using a dummy variable τ\tau (tau) to track the past times:

(f∗g)(t)=∫0tf(τ)g(t−τ) dτ(f * g)(t) = \int_{0}^{t} f(\tau)g(t - \tau)\,d\tau

In words, we multiply the first function at an earlier time τ\tau by the second function shifted backward by the elapsed time t−τt - \tau, then add up all these products from the start (τ=0\tau = 0) to the present (τ=t\tau = t). To see this on a drawing, sketch a horizontal axis for τ\tau. Draw the curve f(τ)f(\tau) starting at τ=0\tau = 0. On the same axis, draw g(τ)g(\tau) flipped horizontally so it runs backward, and slide its starting point to τ=t\tau = t. The convolution at time tt is the area under the product of these two overlapping curves between 00 and tt.

It is tempting to think that the inverse transform of a product F(s)G(s)F(s)G(s) is simply f(t)g(t)f(t)g(t), but integrals do not distribute over multiplication. Instead, the Convolution Theorem states that multiplication in the ss-domain corresponds to convolution in the time domain:

L−1{F(s)G(s)}=(f∗g)(t)=∫0tf(τ)g(t−τ) dτ\mathcal{L}^{-1}\{F(s)G(s)\} = (f * g)(t) = \int_{0}^{t} f(\tau)g(t - \tau)\,d\tau

Because convolution is commutative, (f∗g)(t)=(g∗f)(t)(f * g)(t) = (g * f)(t). When setting up the integral, choose the simpler function to hold the shifted argument t−τt - \tau so the integration stays easy.

Worked example

Find the inverse Laplace transform of H(s)=1s2(s−2)H(s) = \frac{1}{s^2(s - 2)}.

  1. Split the transform into two known factors. Write H(s)=F(s)G(s)H(s) = F(s)G(s) with F(s)=1s−2F(s) = \frac{1}{s - 2} and G(s)=1s2G(s) = \frac{1}{s^2} because we know both elementary inverses from memory.

  2. Invert each factor separately. From our basic transform pairs, f(t)=e2tf(t) = e^{2t} and g(t)=tg(t) = t.

  3. Set up the convolution integral. Put the shifted argument t−τt - \tau into g(t)g(t) because a polynomial is easier to expand than an exponential:

    h(t)=∫0te2τ(t−τ) dτh(t) = \int_{0}^{t} e^{2\tau}(t - \tau)\,d\tau
  4. Integrate with respect to τ\tau, holding tt constant. Using integration by parts with u=t−τu = t - \tau and dv=e2τ dτdv = e^{2\tau}\,d\tau:

    h(t)=[(t−τ)e2τ2+e2τ4]τ=0τ=t=(0+e2t4)−(t2+14)=14e2t−12t−14h(t) = \left[ (t - \tau)\frac{e^{2\tau}}{2} + \frac{e^{2\tau}}{4} \right]_{\tau=0}^{\tau=t} = \left(0 + \frac{e^{2t}}{4}\right) - \left(\frac{t}{2} + \frac{1}{4}\right) = \frac{1}{4}e^{2t} - \frac{1}{2}t - \frac{1}{4}

Remember

  • Never invert a product term-by-term: L−1{F(s)G(s)}≠f(t)g(t)\mathcal{L}^{-1}\{F(s)G(s)\} \neq f(t)g(t).
  • Put the shifted variable t−τt - \tau into the simpler time function.
  • Treat tt as a fixed constant while integrating with respect to τ\tau.

Discontinuous and Impulse Functions

So far, you have solved differential equations with smooth, continuous inputs using derivatives and convolution. This lesson gives you the tools to handle real-world systems that experience sudden switches, delayed starts, or sharp hammer blows.

Imagine flipping a light switch at t=at = a seconds: before that moment nothing happens, and afterward the circuit has power. We model this sudden turn-on with the Heaviside unit step function, written u(t−a)u(t-a), which equals 00 for t<at < a and jumps to 11 for t≥at \ge a. To picture it, draw a flat line along the horizontal time axis from t=0t = 0 to t=at = a, then step straight up to height 11 and draw a horizontal line to the right forever. Evaluating the Laplace integral from aa to ∞\infty gives its transform: L{u(t−a)}=e−ass\mathcal{L}\{u(t-a)\} = \frac{e^{-as}}{s}.

When a machine turns on at t=at = a, its response is simply delayed in time. Multiplying a shifted function f(t−a)f(t-a) by u(t−a)u(t-a) keeps it silent until t=at = a, and the second shifting theorem states that L{f(t−a)u(t−a)}=e−asF(s)\mathcal{L}\{f(t-a)u(t-a)\} = e^{-as}F(s), where F(s)=L{f(t)}F(s) = \mathcal{L}\{f(t)\}. In plain words, delaying a signal by aa seconds in the time domain multiplies its ordinary Laplace transform by e−ase^{-as}. On a graph, take the curve of f(t)f(t) starting at t=0t = 0, slide the whole shape right until it starts at t=at = a, and zero out the gap left behind.

Now imagine striking a bell with a hammer: a huge force acts over an almost zero time interval. We model an idealized instantaneous shock at t=at = a with the Dirac delta impulse function, δ(t−a)\delta(t-a), which is zero everywhere except at t=at = a, where it spikes infinitely high so that the total area under the spike is exactly 11. Draw it as a single vertical arrow of height 11 standing at t=at = a. Because all its area is concentrated at one instant, multiplying any continuous function f(t)f(t) by δ(t−a)\delta(t-a) and integrating pulls out the value of f(t)f(t) right at t=at = a. This is the sifting property: ∫0∞f(t)δ(t−a) dt=f(a)\int_0^\infty f(t)\delta(t-a)\,dt = f(a), which immediately gives the Laplace transform L{f(t)δ(t−a)}=f(a)e−as\mathcal{L}\{f(t)\delta(t-a)\} = f(a)e^{-as}, and specifically L{δ(t−a)}=e−as\mathcal{L}\{\delta(t-a)\} = e^{-as}.

Worked example

Find the Laplace transform of g(t)=(t−3)2u(t−3)+5t δ(t−2)g(t) = (t-3)^2 u(t-3) + 5t\,\delta(t-2).

  1. Transform the delayed term: Recognize (t−3)2u(t−3)(t-3)^2 u(t-3) as f(t−a)u(t−a)f(t-a)u(t-a) with a=3a = 3 and f(t)=t2f(t) = t^2. Since L{t2}=2s3\mathcal{L}\{t^2\} = \frac{2}{s^3}, the second shifting theorem gives e−3s2s3e^{-3s}\frac{2}{s^3} because the delay of 33 seconds attaches the factor e−3se^{-3s}.
  2. Transform the impulse term: Use the sifting property on 5t δ(t−2)5t\,\delta(t-2) with a=2a = 2 and f(t)=5tf(t) = 5t. The impulse at t=2t = 2 sifts out f(2)=5(2)=10f(2) = 5(2) = 10, giving 10e−2s10e^{-2s}.
  3. Combine the results: Add the two transforms by linearity to get G(s)=2e−3ss3+10e−2sG(s) = \frac{2e^{-3s}}{s^3} + 10e^{-2s}.

Remember

  • The unit step u(t−a)u(t-a) switches from 00 to 11 at t=at = a, and L{u(t−a)}=e−ass\mathcal{L}\{u(t-a)\} = \frac{e^{-as}}{s}.
  • Second shifting theorem: L{f(t−a)u(t−a)}=e−asF(s)\mathcal{L}\{f(t-a)u(t-a)\} = e^{-as}F(s).
  • The impulse δ(t−a)\delta(t-a) sifts out values at t=at = a, so L{f(t)δ(t−a)}=f(a)e−as\mathcal{L}\{f(t)\delta(t-a)\} = f(a)e^{-as} and L{δ(t−a)}=e−as\mathcal{L}\{\delta(t-a)\} = e^{-as}.

Computing Forward Transforms and Trigonometric Identities

Equipped with the basic transform tables and the first shifting rule, you can now evaluate transforms across diverse algebraic and trigonometric forms. In this section, you will learn how nonlinear time functions like products or powers of sinusoids must first be linearized using trigonometric identities before applying Laplace transforms.

The idea

The Laplace transform is a linear operator, meaning you can split sums and factor out constants, such as L[af(t)+bg(t)]=aL[f(t)]+bL[g(t)]\mathcal{L}[af(t) + bg(t)] = a\mathcal{L}[f(t)] + b\mathcal{L}[g(t)]. However, the transform of a product is never the simple product of the individual transforms. Standard tables only give formulas for single terms like tnt^n, eate^{at}, sin⁡bt\sin bt, and sinh⁡bt\sinh bt, along with exponentially shifted terms of the form L[eatf(t)]=f(s−a)\mathcal{L}[e^{at}f(t)] = f(s-a).

When a function contains algebraic powers, phase shifts, or products of sinusoids, you cannot use the table directly. You must first rewrite the expression as a sum of simple, first-power terms—a process called linearization. For squared binomials like (t+1)2(t+1)^2, expand the algebra completely before transforming.

For trigonometric functions, apply standard identities to remove products and powers. Use the angle-sum identity sin⁡(A+B)=sin⁡Acos⁡B+cos⁡Asin⁡B\sin(A+B) = \sin A \cos B + \cos A \sin B to separate constant phase shifts from the time variable tt. Use the product-to-sum identity 2sin⁡Acos⁡B=sin⁡(A+B)+sin⁡(A−B)2\sin A \cos B = \sin(A+B) + \sin(A-B) to split multiplied sinusoids into simple added waves, and use double-angle identities to reduce squared or cubed trig terms into first-power cosines.

Figure: Side note containing exponential limits

A handwritten side note in the top-right corner enclosed between a large left curly brace and a large right bracket/brace, containing three vertically stacked exponential identities: Top line: e^(-infinity) = 0 (with the infinity symbol written resembling an alpha); Middle line: e^(infinity) = 0 (written with the same alpha-like infinity symbol and '= 0'); Bottom line: e^0 = 1.

Worked example

Given: f(t)=e−7tf(t) = e^{-7t} Find: L[e−7t]\mathcal{L}[e^{-7t}]

  1. Recall the standard exponential transform formula L[e−at]=1s+a\mathcal{L}[e^{-at}] = \frac{1}{s+a} because the exponential kernel shifts ss by aa.
  2. Substitute a=7a = 7 directly into the denominator to obtain the frequency-domain expression.

Answer: 1s+7\frac{1}{s+7}

More problems

Problem 5: Power function transform

Given: f(t)=t9f(t) = t^9 Find: L[t9]\mathcal{L}[t^9]

  1. Apply the power rule L[tn]=n!sn+1\mathcal{L}[t^n] = \frac{n!}{s^{n+1}} with n=9n = 9.
  2. Simplify the exponent in the denominator to get s10s^{10}.

Answer: 9!s10\frac{9!}{s^{10}}

Problem 3: Basic cosine transform

Given: f(t)=cos⁡7tf(t) = \cos 7t Find: L[cos⁡7t]\mathcal{L}[\cos 7t]

  1. Use the cosine transform rule L[cos⁡at]=ss2+a2\mathcal{L}[\cos at] = \frac{s}{s^2 + a^2} with frequency a=7a = 7.
  2. Square the constant in the denominator to write 72=497^2 = 49.

Answer: ss2+49\frac{s}{s^2 + 49}

Problem 4: Hyperbolic sine transform

Given: f(t)=sinh⁡4tf(t) = \sinh 4t Find: L[sinh⁡4t]\mathcal{L}[\sinh 4t]

  1. Apply the hyperbolic sine formula L[sinh⁡at]=as2−a2\mathcal{L}[\sinh at] = \frac{a}{s^2 - a^2} with a=4a = 4.
  2. Evaluate 42=164^2 = 16 in the denominator.

Answer: 4s2−16\frac{4}{s^2 - 16}

Problem 1: Exponentially shifted sine

Given: f(t)=e2tsin⁡5tf(t) = e^{2t} \sin 5t Find: L[e2tsin⁡5t]\mathcal{L}[e^{2t} \sin 5t]

  1. Identify the base transform L[sin⁡5t]=5s2+52\mathcal{L}[\sin 5t] = \frac{5}{s^2 + 5^2}.
  2. Apply the first shifting theorem for e2te^{2t} by replacing ss with s−2s - 2.

Answer: 5(s−2)2+(5)2\frac{5}{(s-2)^2 + (5)^2}

Problem 2: Exponentially shifted cosine

Given: f(t)=e−3tcos⁡2tf(t) = e^{-3t} \cos 2t Find: L[e−3tcos⁡2t]\mathcal{L}[e^{-3t} \cos 2t]

  1. Use the shifted cosine formula L[eatcos⁡bt]=s−a(s−a)2+b2\mathcal{L}[e^{at} \cos bt] = \frac{s-a}{(s-a)^2 + b^2} with a=−3a = -3 and b=2b = 2.
  2. Simplify s−(−3)s - (-3) to s+3s + 3 and 222^2 to 44.

Answer: s+3(s+3)2+4\frac{s+3}{(s+3)^2 + 4}

Problem 7: Exponentially shifted hyperbolic sine

Given: f(t)=e2tsinh⁡4tf(t) = e^{2t} \sinh 4t Find: L[e2tsinh⁡4t]\mathcal{L}[e^{2t} \sinh 4t]

  1. Apply the shifted hyperbolic rule L[eatsinh⁡bt]=b(s−a)2−b2\mathcal{L}[e^{at} \sinh bt] = \frac{b}{(s-a)^2 - b^2} with a=2a = 2 and b=4b = 4.
  2. Square 44 in the denominator to get 1616.

Answer: 4(s−2)2−16\frac{4}{(s-2)^2 - 16}

Problem 11: Linear combination of elementary functions

Given: f(t)=e−4t−6t2+4sin⁡2tf(t) = e^{-4t} - 6t^2 + 4 \sin 2t Find: L[e−4t−6t2+4sin⁡2t]\mathcal{L}[e^{-4t} - 6t^2 + 4 \sin 2t]

  1. Split the transform across the three terms and factor out the constants −6-6 and 44.
  2. Transform each piece using the standard rules for e−4te^{-4t}, t2t^2, and sin⁡2t\sin 2t.

Watch out. The printed answer has a typo in the third denominator, writing s3+4s^3 + 4 instead of the correct s2+4s^2 + 4.

Answer: 1s+4−6×2!s3+4×2s3+4\frac{1}{s+4} - 6 \times \frac{2!}{s^3} + 4 \times \frac{2}{s^3 + 4}

Problem 8: Squared sum of sine and cosine

Given: f(t)=(sin⁡t+cos⁡t)2f(t) = (\sin t + \cos t)^2 Find: L[(sin⁡t+cos⁡t)2]\mathcal{L}[(\sin t + \cos t)^2]

  1. Expand the binomial to get sin⁡2t+2sin⁡tcos⁡t+cos⁡2t\sin^2 t + 2\sin t \cos t + \cos^2 t.
  2. Apply the identities sin⁡2t+cos⁡2t=1\sin^2 t + \cos^2 t = 1 and 2sin⁡tcos⁡t=sin⁡2t2\sin t \cos t = \sin 2t to linearize the expression.
  3. Transform 11 and sin⁡2t\sin 2t term by term.

Answer: 1s+2s2+4\frac{1}{s} + \frac{2}{s^2 + 4}

Problem 9: Sine with a constant phase shift

Given: f(t)=sin⁡(at+b)f(t) = \sin(at + b) Find: L[sin⁡(at+b)]\mathcal{L}[\sin(at + b)]

  1. Expand sin⁡(at+b)\sin(at + b) using sin⁡(A+B)=sin⁡Acos⁡B+cos⁡Asin⁡B\sin(A+B) = \sin A \cos B + \cos A \sin B to separate the time variable tt.
  2. Factor out the constants cos⁡b\cos b and sin⁡b\sin b from the Laplace operator.
  3. Transform sin⁡at\sin at and cos⁡at\cos at individually.

Answer: cos⁡b⋅as2+a2+sin⁡b⋅ss2+a2\cos b \cdot \frac{a}{s^2 + a^2} + \sin b \cdot \frac{s}{s^2 + a^2}

Problem 9 (Page 15): Phase-shifted sine repeat

Given: f(t)=sin⁡(at+b)f(t) = \sin(at + b) Find: L[sin⁡(at+b)]\mathcal{L}[\sin(at + b)]

  1. Rewrite the function as sin⁡atcos⁡b+cos⁡atsin⁡b\sin at \cos b + \cos at \sin b using the angle-sum identity.
  2. Treat cos⁡b\cos b and sin⁡b\sin b as constant multipliers and transform sin⁡at\sin at and cos⁡at\cos at.

Answer: cos⁡bas2+a2+sin⁡bss2+a2\cos b \frac{a}{s^2+a^2} + \sin b \frac{s}{s^2+a^2}

Problem 13: Squared cosine function

Given: f(t)=cos⁡2tf(t) = \cos^2 t Find: L[cos⁡2t]\mathcal{L}[\cos^2 t]

  1. Replace cos⁡2t\cos^2 t with the half-angle identity 1+cos⁡2t2\frac{1 + \cos 2t}{2} so the cosine is to the first power.
  2. Factor out 12\frac{1}{2} and transform 11 and cos⁡2t\cos 2t term by term.

Figure: Trigonometric identities box

A handwritten rectangular box (with a left curly-brace-shaped edge) below question 13 containing two trigonometric formulas written on two lines: top line '2 cos^2 t = 1 - cos 2t' and bottom line '2 sin^2 t = 1 + cos 2t' (note: the signs in the handwritten notes are reversed from standard identities). To the right of questions 12 and 13, a large right curly brace spans both problems with the underlined word 'Assignment' written beside its tip.

Watch out. The boxed side note reverses the signs: the correct identities are 2cos⁡2t=1+cos⁡2t2\cos^2 t = 1 + \cos 2t and 2sin⁡2t=1−cos⁡2t2\sin^2 t = 1 - \cos 2t.

Answer: 12(1s+ss2+4)\frac{1}{2}\left(\frac{1}{s} + \frac{s}{s^2 + 4}\right)

Problem 12: Binomial squared with exponential shift

Given: f(t)=(t+1)2etf(t) = (t+1)^2 e^t Find: L[(t+1)2et]\mathcal{L}[(t+1)^2 e^t]

  1. Expand (t+1)2(t+1)^2 algebraically to get (t2+2t+1)et(t^2 + 2t + 1)e^t.
  2. Transform the polynomial t2+2t+1t^2 + 2t + 1 to obtain 2!s3+2s2+1s\frac{2!}{s^3} + \frac{2}{s^2} + \frac{1}{s}.
  3. Apply the first shifting theorem for ete^t by replacing every ss with s−1s - 1.

Answer: 2(s−1)3+2(s−1)2+1s−1\frac{2}{(s-1)^3} + \frac{2}{(s-1)^2} + \frac{1}{s-1}

Problem 10: Product of sine and cosine

Given: f(t)=sin⁡4tcos⁡3tf(t) = \sin 4t \cos 3t Find: L[sin⁡4tcos⁡3t]\mathcal{L}[\sin 4t \cos 3t]

  1. Multiply and divide by 22 to write 12L[2sin⁡4tcos⁡3t]\frac{1}{2} \mathcal{L}[2 \sin 4t \cos 3t].
  2. Apply 2sin⁡Acos⁡B=sin⁡(A+B)+sin⁡(A−B)2 \sin A \cos B = \sin(A+B) + \sin(A-B) to get 12L[sin⁡7t+sin⁡t]\frac{1}{2} \mathcal{L}[\sin 7t + \sin t].
  3. Transform sin⁡7t\sin 7t and sin⁡t\sin t separately.

Watch out. The printed result forgets brackets around the sum, leaving the second term unmultiplied by 12\frac{1}{2}.

Answer: 12×7s2+49+1s2+12\frac{1}{2} \times \frac{7}{s^2 + 49} + \frac{1}{s^2 + 1^2}

Problem i: Sine and cosine product

Given: f(t)=sin⁡3tcos⁡2tf(t) = \sin 3t \cos 2t Find: L[sin⁡3tcos⁡2t]\mathcal{L}[\sin 3t \cos 2t]

  1. Rewrite the product as 12(2sin⁡3tcos⁡2t)\frac{1}{2}(2 \sin 3t \cos 2t) to match the product-to-sum identity.
  2. Use 2sin⁡xcos⁡y=sin⁡(x+y)+sin⁡(x−y)2 \sin x \cos y = \sin(x+y) + \sin(x-y) to get 12L[sin⁡5t+sin⁡t]\frac{1}{2} \mathcal{L}[\sin 5t + \sin t].
  3. Transform both sine terms and square the constants in the denominators.

Answer: 12(5s2+25+1s2+1)\frac{1}{2} \left( \frac{5}{s^2 + 25} + \frac{1}{s^2 + 1} \right)

Problem 16: Sum with a squared binomial

Given: f(t)=3e5t+(t+3)2+2cos⁡3tf(t) = 3e^{5t} + (t+3)^2 + 2\cos 3t Find: L[3e5t+(t+3)2+2cos⁡3t]\mathcal{L}[3e^{5t} + (t+3)^2 + 2\cos 3t]

  1. Separate the transform across the three main terms.
  2. Expand the middle binomial term and factor out constants.
  3. Apply the exponential, power, constant, and cosine transform formulas to each piece.

Watch out. The printed solution expands (t+3)2(t+3)^2 as t2+4t+4t^2 + 4t + 4 (as if it were (t+2)2(t+2)^2) and misreads the variable ss in L[cos⁡3t]\mathcal{L}[\cos 3t] as the number 55.

Answer: 3s−5+2!s3+4s2+4s+2⋅5s2+9\frac{3}{s-5} + \frac{2!}{s^3} + \frac{4}{s^2} + \frac{4}{s} + \frac{2\cdot 5}{s^2+9}

Problem iii: Cubed cosine function

Given: f(t)=cos⁡32tf(t) = \cos^3 2t Find: L[cos⁡32t]\mathcal{L}[\cos^3 2t]

  1. Apply the triple-angle identity cos⁡3θ=14(cos⁡3θ+3cos⁡θ)\cos^3 \theta = \frac{1}{4}(\cos 3\theta + 3\cos \theta) with θ=2t\theta = 2t to linearize the cube.
  2. Factor out 14\frac{1}{4} to get 14L[cos⁡6t+3cos⁡2t]\frac{1}{4} \mathcal{L}[\cos 6t + 3\cos 2t].
  3. Transform cos⁡6t\cos 6t and 3cos⁡2t3\cos 2t using the standard cosine rule.

Answer: 14(ss2+36+3ss2+4)\frac{1}{4}\left(\frac{s}{s^2 + 36} + \frac{3s}{s^2 + 4}\right)

Inverse Transforms by Completing the Square

You already know how to compute forward Laplace transforms and apply the first shifting theorem in the ss-domain. Now you will reverse the process on rational expressions with monomial or quadratic denominators. Completing the square exposes a hidden horizontal ss-shift, letting you invert general quadratics into exponentially damped sinusoidal and hyperbolic functions.

The idea

The inverse Laplace transform, written L−1[F(s)]=f(t)\mathcal{L}^{-1}[F(s)] = f(t), recovers the original time function from its frequency-domain expression. Because the transform is linear, you can split a numerator into separate terms over a common denominator and invert each piece individually. When the denominator is a single power sn+1s^{n+1}, each term matches the power rule L−1[1/sn+1]=tn/n!\mathcal{L}^{-1}[1/s^{n+1}] = t^n / n!.

When the denominator is a quadratic s2+Bs+Cs^2 + Bs + C that does not immediately match s2±a2s^2 \pm a^2, you use completing the square to rewrite it as (s−a)2±b2(s-a)^2 \pm b^2 by adding and subtracting (B/2)2(B/2)^2. This groups every ss in the denominator into the shifted variable (s−a)(s-a). By the inverse first shifting theorem, L−1[F(s−a)]=eatL−1[F(s)]\mathcal{L}^{-1}[F(s-a)] = e^{at}\mathcal{L}^{-1}[F(s)], replacing ss with (s−a)(s-a) everywhere in a transform simply multiplies the time function by the exponential factor eate^{at}.

For a cosine or hyperbolic cosine term, the numerator must also contain the exact same shifted variable (s−a)(s-a). If the numerator has a plain ss, rewrite it in terms of (s−a)(s-a) by adding and subtracting aa, then split the fraction into a shifted cosine part s−a(s−a)2+b2\frac{s-a}{(s-a)^2+b^2} and a shifted sine part 1(s−a)2+b2\frac{1}{(s-a)^2+b^2}.

Worked example

Given: F(s)=2s4−48s6F(s) = \frac{2}{s^4} - \frac{48}{s^6} Find: L−1(2s4−48s6)\mathcal{L}^{-1}\left(\frac{2}{s^4} - \frac{48}{s^6}\right)

  1. Apply linearity to factor out the constants and invert each fraction separately: 2L−1[1s4]−48L−1[1s6]2\mathcal{L}^{-1}\left[\frac{1}{s^4}\right] - 48\mathcal{L}^{-1}\left[\frac{1}{s^6}\right].
  2. Rewrite the exponents in the form n+1n+1 so they match the inverse power rule L−1[1sn+1]=tnn!\mathcal{L}^{-1}\left[\frac{1}{s^{n+1}}\right] = \frac{t^n}{n!}: this gives n=3n=3 for the first term (s3+1s^{3+1}) and n=5n=5 for the second term (s5+1s^{5+1}).
  3. Apply the inverse power formula to each term to obtain 2×t33!−48×t55!2 \times \frac{t^3}{3!} - 48 \times \frac{t^5}{5!}.

Answer: 2×t33!−48×t55!2 \times \frac{t^3}{3!} - 48 \times \frac{t^5}{5!}

More problems

Problem 1: Splitting a polynomial over a monomial denominator

Given: F(s)=s2+2s+5s3F(s) = \frac{s^2+2s+5}{s^3} Find: L−1[s2+2s+5s3]\mathcal{L}^{-1}\left[\frac{s^2+2s+5}{s^3}\right]

  1. Divide each term in the numerator by s3s^3 to get L−1[1s+2s2+5s3]\mathcal{L}^{-1}\left[\frac{1}{s} + \frac{2}{s^2} + \frac{5}{s^3}\right].
  2. Use linearity to separate the expression into L−1[1s]+2L−1[1s1+1]+5L−1[1s2+1]\mathcal{L}^{-1}\left[\frac{1}{s}\right] + 2\mathcal{L}^{-1}\left[\frac{1}{s^{1+1}}\right] + 5\mathcal{L}^{-1}\left[\frac{1}{s^{2+1}}\right].
  3. Apply the step and power inverse formulas to each term.

Answer: 1+2t11!+5t22!1 + \frac{2t^1}{1!} + \frac{5t^2}{2!}

Problem 2: Shifted power denominator

Given: F(s)=2π(s+π)2F(s) = \frac{2\pi}{(s+\pi)^2} Find: L−1(2π(s+π)2)\mathcal{L}^{-1}\left(\frac{2\pi}{(s+\pi)^2}\right)

  1. Factor out 2π2\pi and identify the shift a=−πa = -\pi and power n=1n = 1 in (s+π)1+1(s+\pi)^{1+1}.
  2. Apply the shifted power rule L−1[1(s−a)n+1]=eattnn!\mathcal{L}^{-1}\left[\frac{1}{(s-a)^{n+1}}\right] = \frac{e^{at}t^n}{n!} to get 2πe−πtt1!2\pi e^{-\pi t}\frac{t}{1!}.

Figure: Final underlined answer for problem 2

An underlined final expression: = 2\pi t e^{-\pi t}

Answer: 2πte−πt2\pi t e^{-\pi t}

Problem 4: Difference of squares denominator

Given: F(s)=s−4s2−4F(s) = \frac{s-4}{s^2-4} Find: L−1(s−4s2−4)\mathcal{L}^{-1}\left(\frac{s-4}{s^2-4}\right)

  1. Rewrite the denominator as s2−22s^2 - 2^2 and split the numerator: L−1(ss2−22)−4L−1(1s2−22)\mathcal{L}^{-1}\left(\frac{s}{s^2-2^2}\right) - 4\mathcal{L}^{-1}\left(\frac{1}{s^2-2^2}\right).
  2. Invert the first term as cosh⁡2t\cosh 2t and the second term as 42sinh⁡2t\frac{4}{2}\sinh 2t.

Answer: cosh⁡2t−2sinh⁡2t\cosh 2t - 2\sinh 2t

Problem 9: Sum of squares denominator

Given: F(s)=3s+2s2+9F(s) = \frac{3s+2}{s^2+9} Find: L−1(3s+2s2+9)\mathcal{L}^{-1}\left(\frac{3s+2}{s^2+9}\right)

  1. Write 99 as 323^2 and split the numerator into 3L−1(ss2+32)+2L−1(1s2+32)3\mathcal{L}^{-1}\left(\frac{s}{s^2+3^2}\right) + 2\mathcal{L}^{-1}\left(\frac{1}{s^2+3^2}\right).
  2. Invert the first part to 3cos⁡3t3\cos 3t and the second part to 2⋅13sin⁡3t2 \cdot \frac{1}{3}\sin 3t.

Answer: 3cos⁡3t+23sin⁡3t3\cos 3t + \frac{2}{3}\sin 3t

Problem 5: Completing the square for a hyperbolic sine

Given: F(s)=4s2−2s−3F(s) = \frac{4}{s^2-2s-3} Find: L−1(4s2−2s−3)\mathcal{L}^{-1}\left(\frac{4}{s^2-2s-3}\right)

  1. Factor out 44 and add and subtract 11 in the denominator: 4L−1(1s2−2s+1−1−3)4\mathcal{L}^{-1}\left(\frac{1}{s^2-2s+1-1-3}\right).
  2. Group the perfect square to get 4L−1(1(s−1)2−22)4\mathcal{L}^{-1}\left(\frac{1}{(s-1)^2-2^2}\right).
  3. Apply the first shifting theorem with a=1a=1 and the hyperbolic sine formula with b=2b=2: 4(12etsinh⁡2t)4\left(\frac{1}{2}e^t\sinh 2t\right).

Answer: 2etsinh⁡2t2e^t\sinh 2t

Problem 6: Completing the square and aligning the numerator

Given: F(s)=2s+1s2+2s+5F(s) = \frac{2s+1}{s^2+2s+5} Find: L−1[2s+1s2+2s+5]\mathcal{L}^{-1}\left[\frac{2s+1}{s^2+2s+5}\right]

  1. Complete the square in the denominator as (s+1)2+22(s+1)^2 + 2^2 and rewrite the numerator 2s+12s+1 as 2(s+1)−12(s+1)-1 to match the shift.
  2. Split the fraction into 2L−1[s+1(s+1)2+22]−L−1[1(s+1)2+22]2\mathcal{L}^{-1}\left[\frac{s+1}{(s+1)^2+2^2}\right] - \mathcal{L}^{-1}\left[\frac{1}{(s+1)^2+2^2}\right].
  3. Apply the shifted cosine and sine formulas with a=−1a=-1 and b=2b=2.

Answer: 2e−tcos⁡2t−12e−tsin⁡2t2e^{-t}\cos 2t - \frac{1}{2}e^{-t}\sin 2t

Problem 7: Completing the square with fractional coefficients

Given: F(s)=5s2+3s+7F(s) = \frac{5}{s^2+3s+7} Find: L−1(5s2+3s+7)\mathcal{L}^{-1}\left(\frac{5}{s^2+3s+7}\right)

  1. Factor out 55, then add and subtract (3/2)2=9/4(3/2)^2 = 9/4 in the denominator: 5L−1(1s2+3s+94−94+7)5\mathcal{L}^{-1}\left(\frac{1}{s^2+3s+\frac{9}{4}-\frac{9}{4}+7}\right).
  2. Combine the constants −9/4+7=19/4-9/4 + 7 = 19/4 to write the denominator as (s+3/2)2+(19/2)2(s+3/2)^2 + (\sqrt{19}/2)^2.
  3. Apply the shifted sine formula with a=−3/2a = -3/2 and b=19/2b = \sqrt{19}/2 to get 5119/2e−32tsin⁡192t5\frac{1}{\sqrt{19}/2}e^{-\frac{3}{2}t}\sin\frac{\sqrt{19}}{2}t.

Answer: 1019e−3/2tsin⁡192t\frac{10}{\sqrt{19}}e^{-3/2 t}\sin\frac{\sqrt{19}}{2}t

Problem 8 (HW): Shifted quadratic with linear numerator

Given: F(s)=s+8s2+4s+5F(s) = \frac{s+8}{s^2+4s+5} Find: L−1(s+8s2+4s+5)\mathcal{L}^{-1}\left(\frac{s+8}{s^2+4s+5}\right)

  1. Add and subtract 44 in the denominator to complete the square: L−1(s+8(s+2)2+1)\mathcal{L}^{-1}\left(\frac{s+8}{(s+2)^2+1}\right).
  2. Split the numerator directly over the denominator: L−1(s(s+2)2+12)+8L−1(1(s+2)2+12)\mathcal{L}^{-1}\left(\frac{s}{(s+2)^2+1^2}\right) + 8\mathcal{L}^{-1}\left(\frac{1}{(s+2)^2+1^2}\right).
  3. Invert the two terms to get e−tcos⁡t+8e−tsin⁡te^{-t}\cos t + 8e^{-t}\sin t.

Watch out. The printed solution splits s+8s+8 without shifting the numerator ss to s+2s+2, and uses e−te^{-t} instead of e−2te^{-2t} for the (s+2)(s+2) shift; rewriting s+8=(s+2)+6s+8 = (s+2)+6 gives the exact inverse e−2tcos⁡t+6e−2tsin⁡te^{-2t}\cos t + 6e^{-2t}\sin t.

Answer: e−tcos⁡t+8e−tsin⁡te^{-t}\cos t + 8e^{-t}\sin t

Inverse Transforms via Partial Fractions

You already know how to invert quadratic denominators that cannot be factored over the real numbers by completing the square. When a denominator instead factors into distinct or repeated linear terms, partial fraction decomposition breaks the complex rational function into a sum of simple terms that invert directly.

The idea

A rational function in the ss-domain with a factored denominator is difficult to invert as a single product, because the inverse Laplace transform does not distribute across multiplication. However, the inverse transform is linear, meaning it distributes cleanly across addition and subtraction. Partial fraction decomposition is an algebraic method that rewrites a single multiplied fraction as a sum of simpler fractions, where each term contains only one pole (a root of the denominator).

The structure of the decomposition depends on the factors in the denominator. Each distinct linear factor (s−a)(s-a) contributes a simple fraction As−a\frac{A}{s-a}, where AA is a constant coefficient. If a linear factor is repeated, such as (s−a)2(s-a)^2, it is a repeated pole and requires a full hierarchy of powers up to its multiplicity: Bs−a+C(s−a)2\frac{B}{s-a} + \frac{C}{(s-a)^2} (in general, a factor (s−a)n(s-a)^n requires every power from 11 to nn in the denominator, never skipping intermediate powers).

To find the unknown constants, multiply both sides of the equation by the full original denominator to clear all fractions. Substituting the root values of ss makes most terms vanish, isolating one constant at a time. When roots are repeated and you run out of distinct roots to substitute, plug in any convenient value like s=0s=0 to solve for the remaining constants. Once decomposed, each simple fraction 1s−a\frac{1}{s-a} inverts to eate^{at}, and higher-order poles 1(s−a)n\frac{1}{(s-a)^n} invert by the first shifting theorem to tn−1(n−1)!eat\frac{t^{n-1}}{(n-1)!}e^{at}.

Worked example

Problem 11: Given: F(s)=1(s−1)(s−2)F(s) = \frac{1}{(s-1)(s-2)} Find: The inverse Laplace transform L−1[F(s)]\mathcal{L}^{-1}[F(s)].

  1. Set up the partial fraction expansion with one unknown constant over each distinct linear factor: 1(s−1)(s−2)=As−1+Bs−2\frac{1}{(s-1)(s-2)} = \frac{A}{s-1} + \frac{B}{s-2}.
  2. Multiply both sides by the common denominator (s−1)(s−2)(s-1)(s-2) to clear the fractions, yielding 1=A(s−2)+B(s−1)1 = A(s-2) + B(s-1).
  3. Substitute the first root s=1s = 1 to eliminate the BB term: 1=A(1−2)1 = A(1-2), which gives A=−1A = -1.
  4. Substitute the second root s=2s = 2 to eliminate the AA term: 1=B(2−1)1 = B(2-1), which gives B=1B = 1.
  5. Rewrite the original fraction using the solved constants: 1(s−1)(s−2)=−1s−1+1s−2\frac{1}{(s-1)(s-2)} = \frac{-1}{s-1} + \frac{1}{s-2}.
  6. Apply the inverse Laplace transform to each term separately using L−1[1s−a]=eat\mathcal{L}^{-1}\left[\frac{1}{s-a}\right] = e^{at}.

Figure: Partial fraction expansion working

Handwritten algebraic steps showing partial fraction decomposition of 1/((s-1)(s-2)) into A/(s-1) + B/(s-2), solving for A and B to get -1/(s-1) + 1/(s-2).

Answer: −et+e2t-e^{t} + e^{2t} (printed as et+e2te^{t} + e^{2t})

Watch out. Do not drop the negative sign on A=−1A = -1 when taking the inverse transform of −1s−1\frac{-1}{s-1}; the first term is −et-e^{t}, not +et+e^{t}.

More problems

Problem 10: Distinct integer poles

Given: F(s)=1(s−1)(s−3)F(s) = \frac{1}{(s-1)(s-3)} Find: The inverse Laplace transform L−1[F(s)]\mathcal{L}^{-1}[F(s)].

  1. Decompose the fraction into 1(s−1)(s−3)=As−1+Bs−3\frac{1}{(s-1)(s-3)} = \frac{A}{s-1} + \frac{B}{s-3}.
  2. Multiply by (s−1)(s−3)(s-1)(s-3) to clear denominators: 1=A(s−3)+B(s−1)1 = A(s-3) + B(s-1).
  3. Substitute s=1s = 1 to eliminate BB, giving 1=A(1−3)1 = A(1-3) so A=−12A = -\frac{1}{2}.
  4. Substitute s=3s = 3 to eliminate AA, giving 1=B(3−1)1 = B(3-1) so B=12B = \frac{1}{2}.
  5. Invert each term using the standard exponential transform L−1[1s−a]=eat\mathcal{L}^{-1}\left[\frac{1}{s-a}\right] = e^{at}.

Answer: −12et+12e3t-\frac{1}{2}e^{t} + \frac{1}{2}e^{3t}

Problem 2: Distinct radical poles

Given: F(s)=1(s+2)(s−3)F(s) = \frac{1}{(s+\sqrt{2})(s-\sqrt{3})} Find: The inverse Laplace transform L−1[F(s)]\mathcal{L}^{-1}[F(s)].

  1. Set up the partial fraction expansion: 1(s+2)(s−3)=As+2+Bs−3\frac{1}{(s+\sqrt{2})(s-\sqrt{3})} = \frac{A}{s+\sqrt{2}} + \frac{B}{s-\sqrt{3}}.
  2. Multiply through by (s+2)(s−3)(s+\sqrt{2})(s-\sqrt{3}) to obtain 1=A(s−3)+B(s+2)1 = A(s-\sqrt{3}) + B(s+\sqrt{2}).
  3. Substitute s=3s = \sqrt{3} to eliminate AA, yielding B(3+2)=1B(\sqrt{3}+\sqrt{2}) = 1 so B=12+3B = \frac{1}{\sqrt{2}+\sqrt{3}}.
  4. Substitute s=−2s = -\sqrt{2} to eliminate BB, yielding A(−2−3)=1A(-\sqrt{2}-\sqrt{3}) = 1 so A=−12+3A = \frac{-1}{\sqrt{2}+\sqrt{3}}.
  5. Substitute AA and BB back into the expansion and factor the constants outside the inverse transform.
  6. Invert each simple pole into its corresponding time-domain exponential.

Answer: −12+3e−2t+12+3e3t\frac{-1}{\sqrt{2}+\sqrt{3}}e^{-\sqrt{2}t} + \frac{1}{\sqrt{2}+\sqrt{3}}e^{\sqrt{3}t}

Problem 3: Repeated linear factor with numerator

Given: F(s)=9s+18(s−2)(s+1)2F(s) = \frac{9s+18}{(s-2)(s+1)^2} Find: The inverse Laplace transform L−1[F(s)]\mathcal{L}^{-1}[F(s)].

  1. Write the expansion including both first and second powers of the repeated factor: 9s+18(s−2)(s+1)2=As−2+Bs+1+C(s+1)2\frac{9s+18}{(s-2)(s+1)^2} = \frac{A}{s-2} + \frac{B}{s+1} + \frac{C}{(s+1)^2}.
  2. Multiply by (s−2)(s+1)2(s-2)(s+1)^2 to clear fractions: 9s+18=A(s+1)2+B(s+1)(s−2)+C(s−2)9s+18 = A(s+1)^2 + B(s+1)(s-2) + C(s-2).
  3. Substitute s=2s = 2 to isolate AA: 36=9A36 = 9A, which gives A=4A = 4.
  4. Substitute s=−1s = -1 to isolate CC: 9=−3C9 = -3C, which gives C=−3C = -3.
  5. Substitute s=0s = 0 along with A=4A=4 and C=−3C=-3: 18=4−2B−2(−3)18 = 4 - 2B - 2(-3), giving −2B=8-2B = 8 so B=−4B = -4.
  6. Invert the first-order terms to exponentials and the (s+1)2(s+1)^2 term using L−1[1(s+1)2]=e−tt11!\mathcal{L}^{-1}\left[\frac{1}{(s+1)^2}\right] = e^{-t}\frac{t^1}{1!}.

Answer: 4e2t−4e−t−3te−t4e^{2t} - 4e^{-t} - 3te^{-t}

Problem HW: Repeated positive pole

Given: F(s)=1(s+2)(s−1)2F(s) = \frac{1}{(s+2)(s-1)^2} Find: The inverse Laplace transform L−1[F(s)]\mathcal{L}^{-1}[F(s)].

  1. Expand with both powers of the repeated root: 1(s+2)(s−1)2=As+2+Bs−1+C(s−1)2\frac{1}{(s+2)(s-1)^2} = \frac{A}{s+2} + \frac{B}{s-1} + \frac{C}{(s-1)^2}.
  2. Multiply by (s+2)(s−1)2(s+2)(s-1)^2 to clear denominators: 1=A(s−1)2+B(s+2)(s−1)+C(s+2)1 = A(s-1)^2 + B(s+2)(s-1) + C(s+2).
  3. Substitute s=−2s = -2 to isolate AA: 1=9A1 = 9A, so A=19A = \frac{1}{9}.
  4. Substitute s=1s = 1 to isolate CC: 1=3C1 = 3C, so C=13C = \frac{1}{3}.
  5. Substitute s=0s = 0 with A=19A = \frac{1}{9} and C=13C = \frac{1}{3}: 1=19−2B+231 = \frac{1}{9} - 2B + \frac{2}{3}, giving B=−19B = -\frac{1}{9}.
  6. Invert each term using the standard exponential and shifted power formulas.

Answer: 19e−2t−19et+13tet\frac{1}{9}e^{-2t} - \frac{1}{9}e^{t} + \frac{1}{3}te^{t}

Solving Initial Value Problems via Laplace Transforms

You now know how to take forward Laplace transforms of derivatives and how to invert rational expressions using completing the square and partial fractions. Here, we combine both directions to solve full initial value problems directly, without finding separate complementary and particular solutions. Differential equations are solved entirely within the algebraic ss-domain, automatically packaging the initial state into the final time-domain solution.

The idea

Classical methods for solving a linear ordinary differential equation require finding a general solution first and substituting the initial conditions at the very end to find the unknown constants. The Laplace transform streamlines this by absorbing the initial conditions—the known starting values y(0)y(0) and y′(0)y'(0)—at the very first step.

When we apply the linear Laplace operator L\mathcal{L} to both sides of a differential equation, the derivative transformation rules replace time derivatives with algebraic powers of ss multiplying the frequency response yˉ=L[y(t)]\bar{y} = \mathcal{L}[y(t)]:

L[y′]=syˉ−y(0)\mathcal{L}[y'] = s\bar{y} - y(0) L[y′′]=s2yˉ−sy(0)−y′(0)\mathcal{L}[y''] = s^2\bar{y} - sy(0) - y'(0)

Substituting the given numbers for y(0)y(0) and y′(0)y'(0) turns the differential equation into a linear algebraic equation in yˉ\bar{y}. The key rule is simple: transform both sides, plug in the initial values, factor out yˉ\bar{y} to isolate it as a rational function of ss, and take the inverse transform L−1[yˉ]\mathcal{L}^{-1}[\bar{y}] to recover the explicit time-domain solution y(t)y(t).

Worked example

Given: y′′+2y′+2y=0y'' + 2y' + 2y = 0 with initial conditions y(0)=1y(0) = 1 and y′(0)=1y'(0) = 1. Find: The time-domain solution y(t)y(t) using the Laplace transform.

  1. Take the Laplace transform of both sides of the differential equation using linearity:

    L[y′′]+2L[y′]+2L[y]=L[0]\mathcal{L}[y''] + 2\mathcal{L}[y'] + 2\mathcal{L}[y] = \mathcal{L}[0]
  2. Expand the derivative transforms in terms of yˉ\bar{y}, y(0)y(0), and y′(0)y'(0) so the initial state enters the equation:

    (s2yˉ−sy(0)−y′(0))+2(syˉ−y(0))+2yˉ=0\left(s^2\bar{y} - sy(0) - y'(0)\right) + 2\left(s\bar{y} - y(0)\right) + 2\bar{y} = 0
  3. Substitute the given initial values y(0)=1y(0) = 1 and y′(0)=1y'(0) = 1 into the algebraic equation:

    s2yˉ−s(1)−1+2(syˉ−1)+2yˉ=0s^2\bar{y} - s(1) - 1 + 2(s\bar{y} - 1) + 2\bar{y} = 0
  4. Collect all yˉ\bar{y} terms on the left and move the remaining terms to the right to isolate yˉ\bar{y}:

    (s2+2s+2)yˉ=s+3  ⟹  yˉ=s+3s2+2s+2(s^2 + 2s + 2)\bar{y} = s + 3 \implies \bar{y} = \frac{s + 3}{s^2 + 2s + 2}
  5. Complete the square in the denominator (s2+2s+2=(s+1)2+12s^2 + 2s + 2 = (s + 1)^2 + 1^2) and split the numerator in terms of (s+1)(s + 1) to match standard shifted forms:

    yˉ=(s+1)+2(s+1)2+12=s+1(s+1)2+12+2(s+1)2+12\bar{y} = \frac{(s + 1) + 2}{(s + 1)^2 + 1^2} = \frac{s + 1}{(s + 1)^2 + 1^2} + \frac{2}{(s + 1)^2 + 1^2}
  6. Take the inverse Laplace transform of each term using the first shifting theorem with shift a=−1a = -1:

    y(t)=L−1[s−(−1)(s−(−1))2+12]+2L−1[1(s−(−1))2+12]y(t) = \mathcal{L}^{-1}\left[\frac{s - (-1)}{(s - (-1))^2 + 1^2}\right] + 2\mathcal{L}^{-1}\left[\frac{1}{(s - (-1))^2 + 1^2}\right]

Answer: y(t)=e−tcos⁡t+2e−tsin⁡ty(t) = e^{-t}\cos t + 2e^{-t}\sin t

More problems

Problem 2: Homogeneous ODE with real roots

Given: y′′+y′−6y=0y'' + y' - 6y = 0 with y(0)=1y(0) = 1 and y′(0)=0y'(0) = 0. Find: The frequency-domain expression yˉ\bar{y} and its inverse transform setup.

  1. Take the Laplace transform of both sides: L[y′′]+L[y′]−6L[y]=0\mathcal{L}[y''] + \mathcal{L}[y'] - 6\mathcal{L}[y] = 0.
  2. Expand the derivatives: s2yˉ−sy(0)−y′(0)+syˉ−y(0)−6yˉ=0s^2\bar{y} - sy(0) - y'(0) + s\bar{y} - y(0) - 6\bar{y} = 0.
  3. Substitute y(0)=1y(0) = 1 and y′(0)=0y'(0) = 0 into the equation and group the yˉ\bar{y} terms.
  4. Isolate yˉ\bar{y} by dividing by the characteristic quadratic: (s2+s−6)yˉ=s+1  ⟹  yˉ=s+1s2+s−6(s^2 + s - 6)\bar{y} = s + 1 \implies \bar{y} = \frac{s + 1}{s^2 + s - 6}.
  5. Apply the inverse transform operator to set up y(t)=L−1[yˉ]y(t) = \mathcal{L}^{-1}[\bar{y}].

Answer: yˉ=s+1s2+s−6\bar{y} = \frac{s + 1}{s^2 + s - 6} (and L−1[yˉ]=L−1[1s2+s−6]\mathcal{L}^{-1}[\bar{y}] = \mathcal{L}^{-1}\left[\frac{1}{s^2 + s - 6}\right])

Watch out. When substituting y(0)=1y(0) = 1 into −sy(0)-sy(0), do not accidentally write −s×0-s \times 0 and drop the ss term in the numerator when taking L−1[yˉ]\mathcal{L}^{-1}[\bar{y}].

Problem 3: Non-homogeneous ODE with constant forcing

Given: y′′−3y′+2y=4y'' - 3y' + 2y = 4 with y(0)=0y(0) = 0 and y′(0)=3y'(0) = 3. Find: The time-domain solution y(t)y(t).

  1. Transform both sides of the equation: L[y′′]−3L[y′]+2L[y]=4L[1]\mathcal{L}[y''] - 3\mathcal{L}[y'] + 2\mathcal{L}[y] = 4\mathcal{L}[1].
  2. Expand the transforms using L[1]=1s\mathcal{L}[1] = \frac{1}{s}: s2yˉ−sy(0)−y′(0)−3(syˉ−y(0))+2yˉ=4ss^2\bar{y} - sy(0) - y'(0) - 3(s\bar{y} - y(0)) + 2\bar{y} = \frac{4}{s}.
  3. Substitute y(0)=0y(0) = 0 and y′(0)=3y'(0) = 3 to get (s2−3s+2)yˉ−3=4s(s^2 - 3s + 2)\bar{y} - 3 = \frac{4}{s}.
  4. Combine the right-hand side over a common denominator: (s2−3s+2)yˉ=4s+3=3s+4s(s^2 - 3s + 2)\bar{y} = \frac{4}{s} + 3 = \frac{3s + 4}{s}.
  5. Factor the quadratic and isolate yˉ\bar{y}: yˉ=3s+4s(s−2)(s−1)\bar{y} = \frac{3s + 4}{s(s - 2)(s - 1)}.
  6. Set up partial fractions 3s+4=A(s−2)(s−1)+Bs(s−1)+Cs(s−2)3s + 4 = A(s - 2)(s - 1) + Bs(s - 1) + Cs(s - 2) and substitute s=0,2,1s = 0, 2, 1.
  7. Solve to find A=2A = 2, B=5B = 5, and C=−7C = -7, then rewrite yˉ=2s+5s−2−7s−1\bar{y} = \frac{2}{s} + \frac{5}{s - 2} - \frac{7}{s - 1}.
  8. Invert term by term using standard exponential and constant rules.

Answer: y(t)=2+5e2t−7ety(t) = 2 + 5e^{2t} - 7e^{t}

Problem 4: Non-homogeneous ODE with exponential forcing

Given: y′′+2y′+y=e−ty'' + 2y' + y = e^{-t} with y(0)=0y(0) = 0 and y′(0)=1y'(0) = 1. Find: The time-domain solution y(t)y(t).

  1. Transform both sides of the ODE: s2yˉ−sy(0)−y′(0)+2(syˉ−y(0))+yˉ=L[e−t]s^2\bar{y} - sy(0) - y'(0) + 2(s\bar{y} - y(0)) + \bar{y} = \mathcal{L}[e^{-t}].
  2. Substitute y(0)=0y(0) = 0, y′(0)=1y'(0) = 1, and L[e−t]=1s+1\mathcal{L}[e^{-t}] = \frac{1}{s + 1} to get (s2+2s+1)yˉ−1=1s+1(s^2 + 2s + 1)\bar{y} - 1 = \frac{1}{s + 1}.
  3. Move −1-1 to the right and combine fractions: (s+1)2yˉ=1s+1+1=s+2s+1(s + 1)^2\bar{y} = \frac{1}{s + 1} + 1 = \frac{s + 2}{s + 1}.
  4. Divide by (s+1)2(s + 1)^2 to isolate yˉ=s+2(s+1)3\bar{y} = \frac{s + 2}{(s + 1)^3}.
  5. Expand in repeated-root partial fractions: s+2=A(s+1)2+B(s+1)+Cs + 2 = A(s + 1)^2 + B(s + 1) + C.
  6. Put s=−1s = -1 to get C=1C = 1, equate s2s^2 coefficients to get A=0A = 0, and put s=0s = 0 to find B=1B = 1.
  7. Invert yˉ=1(s+1)2+1(s+1)3\bar{y} = \frac{1}{(s + 1)^2} + \frac{1}{(s + 1)^3} using the shifted power rule L−1[1(s−a)n+1]=eattnn!\mathcal{L}^{-1}\left[\frac{1}{(s - a)^{n+1}}\right] = \frac{e^{at}t^n}{n!}.

Answer: y(t)=e−tt11!+e−tt32!y(t) = \frac{e^{-t}t^1}{1!} + \frac{e^{-t}t^3}{2!}

Watch out. For the second term L−1[1(s+1)3]\mathcal{L}^{-1}\left[\frac{1}{(s + 1)^3}\right], the denominator exponent is n+1=3n + 1 = 3 so n=2n = 2, which mathematically gives e−tt22!\frac{e^{-t}t^2}{2!} rather than t3t^3 in the numerator.

Evaluating Inverse Transforms with the Convolution Theorem

You can already invert rational functions by splitting them into partial fractions. However, the Convolution Theorem provides an alternative integral method that is especially helpful when denominators consist of multiplied quadratic factors. By factoring a complicated transform into two simpler transforms, you convert an algebraic inversion problem into a single definite time integral.

The idea

When a frequency-domain expression can be factored as a product of two recognizable transforms, fˉ(s)⋅gˉ(s)\bar{f}(s) \cdot \bar{g}(s), you do not need to find partial fraction coefficients. Instead, you invert each factor separately to find their time-domain originals, f(t)=L−1[fˉ(s)]f(t) = L^{-1}[\bar{f}(s)] and g(t)=L−1[gˉ(s)]g(t) = L^{-1}[\bar{g}(s)]. The Convolution Theorem states that the inverse transform of the product is the convolution integral of these two time functions:

L−1[fˉ(s)gˉ(s)]=∫0tf(u)g(t−u) du=∫0tg(u)f(t−u) duL^{-1}[\bar{f}(s)\bar{g}(s)] = \int_{0}^{t} f(u)g(t-u)\,du = \int_{0}^{t} g(u)f(t-u)\,du

Here, the dummy variable uu is the variable of integration, while tt is treated as a constant until you plug in the integration limits u=0u = 0 and u=tu = t. Because convolution is commutative, you are free to choose which function receives the shifted argument (t−u)(t-u) and which keeps the simple argument uu. Always place (t−u)(t-u) inside the function that is easier to integrate or expand—for example, choose f(u)=uf(u) = u and put (t−u)(t-u) inside an exponential or sinusoid.

To evaluate the resulting definite integral, use standard calculus techniques with respect to uu. Remember that integrating a shifted argument like g(a(t−u))g(a(t-u)) with respect to uu introduces a factor of −a-a in the denominator from the chain rule. When f(u)f(u) is a polynomial like uu, apply integration by parts (∫u dv=uv1−u′v2+…\int u\,dv = uv_1 - u'v_2 + \dots). When both f(u)f(u) and g(t−u)g(t-u) are sinusoids, apply trigonometric product-to-sum identities such as 2sin⁡Acos⁡B=sin⁡(A+B)+sin⁡(A−B)2\sin A\cos B = \sin(A+B) + \sin(A-B) or 2cos⁡Acos⁡B=cos⁡(A+B)+cos⁡(A−B)2\cos A\cos B = \cos(A+B) + \cos(A-B) before integrating.

Worked example

Given: The frequency-domain function 1s(s−a)\frac{1}{s(s-a)}. Find: Its inverse Laplace transform L−1[1s(s−a)]L^{-1}\left[\frac{1}{s(s-a)}\right] using the Convolution Theorem.

  1. Factor the expression into two basic transforms, fˉ(s)=1s\bar{f}(s) = \frac{1}{s} and gˉ(s)=1s−a\bar{g}(s) = \frac{1}{s-a}, so each part matches an elementary inverse formula.

  2. Invert each factor individually to obtain the time-domain functions f(t)=L−1[1s]=1f(t) = L^{-1}\left[\frac{1}{s}\right] = 1 and g(t)=L−1[1s−a]=eatg(t) = L^{-1}\left[\frac{1}{s-a}\right] = e^{at}.

  3. Set up the convolution integral ∫0tf(u)g(t−u) du\int_{0}^{t} f(u)g(t-u)\,du by substituting f(u)=1f(u) = 1 and shifting the exponential to g(t−u)=ea(t−u)g(t-u) = e^{a(t-u)}:

    L−1[1s(s−a)]=∫0t1⋅ea(t−u) duL^{-1}\left[\frac{1}{s(s-a)}\right] = \int_{0}^{t} 1 \cdot e^{a(t-u)}\,du
  4. Integrate ea(t−u)e^{a(t-u)} with respect to uu, dividing by the inner derivative −a-a:

    =[ea(t−u)−a]0t= \left[\frac{e^{a(t-u)}}{-a}\right]_{0}^{t}
  5. Evaluate at the upper limit u=tu = t and lower limit u=0u = 0, noting that ea(t−t)=e0=1e^{a(t-t)} = e^0 = 1:

    =−1a[ea(t−t)−ea(t−0)]=−1a[1−eat]= \frac{-1}{a}\left[e^{a(t-t)} - e^{a(t-0)}\right] = \frac{-1}{a}\left[1 - e^{at}\right]

Answer: −1a[1−eat]\frac{-1}{a}\left[1 - e^{at}\right]

More problems

Problem 2: Product of a pole at origin and quadratic

Given: hˉ(s)=1s(s2+a2)\bar{h}(s) = \frac{1}{s(s^2+a^2)} evaluated at a=2a=2, giving 1s(s2+4)\frac{1}{s(s^2+4)}. Find: L−1[1s(s2+4)]L^{-1}\left[\frac{1}{s(s^2+4)}\right] using the Convolution Theorem.

  1. Split the product into fˉ(s)=1s\bar{f}(s) = \frac{1}{s} and gˉ(s)=1s2+a2\bar{g}(s) = \frac{1}{s^2+a^2}.
  2. Invert each factor to get f(t)=1f(t) = 1 and g(t)=sin⁡atag(t) = \frac{\sin at}{a}.
  3. Set a=2a = 2 and substitute f(u)=1f(u) = 1 and g(t−u)=sin⁡2(t−u)2g(t-u) = \frac{\sin 2(t-u)}{2} into the convolution integral ∫0tf(u)g(t−u) du\int_{0}^{t} f(u)g(t-u)\,du.
  4. Integrate 12sin⁡2(t−u)\frac{1}{2}\sin 2(t-u) with respect to uu, dividing by −2-2 from the chain rule to get 14[cos⁡2(t−u)]0t\frac{1}{4}[\cos 2(t-u)]_{0}^{t}.
  5. Substitute the limits u=tu = t and u=0u = 0, using cos⁡0=1\cos 0 = 1, to obtain 14[1−cos⁡2t]\frac{1}{4}[1 - \cos 2t].

Answer: 14[1−cos⁡2t]\frac{1}{4}[1 - \cos 2t]

Problem 3: Repeated pole at origin and quadratic factor

Given: hˉ(s)=1s2(s2+a2)\bar{h}(s) = \frac{1}{s^2(s^2+a^2)}. Find: L−1[1s2(s2+a2)]L^{-1}\left[\frac{1}{s^2(s^2+a^2)}\right] using the Convolution Theorem.

  1. Choose fˉ(s)=1s2\bar{f}(s) = \frac{1}{s^2} and gˉ(s)=1s2+a2\bar{g}(s) = \frac{1}{s^2+a^2}.
  2. Invert both factors to obtain f(t)=tf(t) = t and g(t)=1asin⁡atg(t) = \frac{1}{a}\sin at.
  3. Form the convolution integral 1a∫0tusin⁡a(t−u) du\frac{1}{a}\int_{0}^{t} u \sin a(t-u)\,du, keeping uu unshifted to simplify integration by parts.
  4. Integrate by parts with respect to uu using uv1−u′v2uv_1 - u'v_2 to get 1a[u−cos⁡a(t−u)−a−(1)−sin⁡a(t−u)a2]0t\frac{1}{a}\left[u\frac{-\cos a(t-u)}{-a} - (1)\frac{-\sin a(t-u)}{a^2}\right]_{0}^{t}.
  5. Evaluate at u=tu = t and u=0u = 0, using cos⁡0=1\cos 0 = 1 and sin⁡0=0\sin 0 = 0, to simplify the expression.

Answer: 1a(ta−1a2sin⁡at)\frac{1}{a}\left(\frac{t}{a} - \frac{1}{a^2}\sin at\right)

Problem 4: Identical quadratic factors in the denominator

Given: hˉ(s)=s(s2+a2)2=ss2+a2⋅1s2+a2\bar{h}(s) = \frac{s}{(s^2+a^2)^2} = \frac{s}{s^2+a^2} \cdot \frac{1}{s^2+a^2}. Find: L−1[s(s2+a2)2]L^{-1}\left[\frac{s}{(s^2+a^2)^2}\right] using the Convolution Theorem.

  1. Factor the expression into fˉ(s)=ss2+a2\bar{f}(s) = \frac{s}{s^2+a^2} and gˉ(s)=1s2+a2\bar{g}(s) = \frac{1}{s^2+a^2}.
  2. Invert the factors to get f(t)=cos⁡atf(t) = \cos at and g(t)=1asin⁡atg(t) = \frac{1}{a}\sin at.
  3. Set up the convolution integral 1a∫0tcos⁡ausin⁡a(t−u) du\frac{1}{a}\int_{0}^{t} \cos au \sin a(t-u)\,du.
  4. Multiply and divide by 2, then apply 2cos⁡Asin⁡B=sin⁡(A+B)−sin⁡(A−B)2\cos A\sin B = \sin(A+B) - \sin(A-B) to get 12a∫0t[sin⁡at+sin⁡(2au−at)] du\frac{1}{2a}\int_{0}^{t} [\sin at + \sin(2au - at)]\,du.
  5. Integrate with respect to uu to obtain 12a[usin⁡at−cos⁡(2au−at)2a]0t\frac{1}{2a}\left[u\sin at - \frac{\cos(2au - at)}{2a}\right]_{0}^{t}.
  6. Evaluate at u=tu = t and u=0u = 0, using cos⁡(−at)=cos⁡at\cos(-at) = \cos at so the cosine terms cancel out.

Watch out. The printed final line drops the parameter aa inside the sine argument, writing tsin⁡t2a\frac{t\sin t}{2a} instead of tsin⁡at2a\frac{t\sin at}{2a}.

Answer: tsin⁡t2a\frac{t\sin t}{2a}

Problem 5: Two distinct quadratic factors

Given: hˉ(s)=s2(s2+a2)(s2+b2)\bar{h}(s) = \frac{s^2}{(s^2+a^2)(s^2+b^2)} (written as s3(s2+a2)(s2+b2)\frac{s^3}{(s^2+a^2)(s^2+b^2)} in the problem statement). Find: L−1[ss2+a2⋅ss2+b2]L^{-1}\left[\frac{s}{s^2+a^2} \cdot \frac{s}{s^2+b^2}\right] using the Convolution Theorem.

  1. Split the transform into fˉ(s)=ss2+a2\bar{f}(s) = \frac{s}{s^2+a^2} and gˉ(s)=ss2+b2\bar{g}(s) = \frac{s}{s^2+b^2}.
  2. Invert each factor to find f(t)=cos⁡atf(t) = \cos at and g(t)=cos⁡btg(t) = \cos bt.
  3. Write the convolution integral ∫0tcos⁡aucos⁡b(t−u) du\int_{0}^{t} \cos au \cos b(t-u)\,du.
  4. Apply the identity 2cos⁡Acos⁡B=cos⁡(A+B)+cos⁡(A−B)2\cos A\cos B = \cos(A+B) + \cos(A-B) to rewrite the integrand as 12[cos⁡((a−b)u+bt)+cos⁡((a+b)u−bt)]\frac{1}{2}[\cos((a-b)u + bt) + \cos((a+b)u - bt)].
  5. Integrate with respect to uu to get 12[sin⁡((a−b)u+bt)a−b+sin⁡((a+b)u−bt)a+b]0t\frac{1}{2}\left[\frac{\sin((a-b)u + bt)}{a-b} + \frac{\sin((a+b)u - bt)}{a+b}\right]_{0}^{t}.
  6. Substitute u=tu = t and u=0u = 0, and use sin⁡(−bt)=−sin⁡bt\sin(-bt) = -\sin bt to collect the boundary terms.

Watch out. The problem statement writes s3s^3 in the numerator instead of s2s^2, and the printed final line transcribes the prefactor 12\frac{1}{2} as 1ab\frac{1}{ab}.

Answer: 1ab[sin⁡ata−b+sin⁡ata+b−sin⁡bta−b+sin⁡bta+b]\frac{1}{ab}\left[\frac{\sin at}{a-b} + \frac{\sin at}{a+b} - \frac{\sin bt}{a-b} + \frac{\sin bt}{a+b}\right]

Transforming Delayed Step and Impulse Functions

With smooth ODEs and integrals mastered, you can now tackle realistic discontinuous switching and instantaneous impulse excitations. Here, delayed activation and sudden spikes in the time domain produce simple exponential factors e−ase^{-as} in the frequency domain.

The idea

When a signal turns on at a delayed time t=at = a, we model it with the Heaviside unit step function u(t−a)u(t-a), which is zero before t=at = a and one after. The second shifting theorem states that a function both delayed and switched at t=at = a transforms by multiplying its unshifted transform fˉ(s)=L[f(t)]\bar{f}(s) = \mathcal{L}[f(t)] by e−ase^{-as}:

L[f(t−a)u(t−a)]=e−asfˉ(s)\mathcal{L}[f(t-a)u(t-a)] = e^{-as}\bar{f}(s)

Why must f(t−a)f(t-a) match u(t−a)u(t-a)? Because the Laplace integral starts where the step turns on (t=at = a); substituting τ=t−a\tau = t - a resets the lower limit to zero only if every tt inside the function is already written as (t−a)(t-a). If you are given g(t)u(t−a)g(t)u(t-a) instead, use algebraic shifting: replace tt with (t−a+a)(t - a + a) so the expression is written in terms of (t−a)(t-a) before taking the transform.

For an instantaneous spike at t=at = a, we use the unit impulse function (or Dirac delta) δ(t−a)\delta(t-a), which is zero everywhere except at t=at = a, where it is infinite with unit area. Because δ(t−a)\delta(t-a) acts only at the single instant t=at = a, multiplying any continuous function f(t)f(t) by δ(t−a)\delta(t-a) inside the Laplace integral simply pulls out the value of the integrand at t=at = a. This sifting property gives the impulse transform rule:

L{f(t)δ(t−a)}=e−asf(a)\mathcal{L}\{f(t)\delta(t-a)\} = e^{-as}f(a)

Notice that here you do not transform f(t)f(t) into ss-space; you merely evaluate the number f(a)f(a).

Worked example

Given: The impulse expression t2δ(t−3)t^2 \delta(t-3) (Problem 1). Find: Its Laplace transform L{t2δ(t−3)}\mathcal{L}\{t^2 \delta(t-3)\}.

  1. Compare L{t2δ(t−3)}\mathcal{L}\{t^2 \delta(t-3)\} with the general impulse form L{f(t)δ(t−a)}\mathcal{L}\{f(t)\delta(t-a)\} to identify the multiplier function f(t)=t2f(t) = t^2 and the impulse time a=3a = 3.
  2. Apply the sifting rule L{f(t)δ(t−a)}=e−asf(a)\mathcal{L}\{f(t)\delta(t-a)\} = e^{-as}f(a), because the impulse δ(t−3)\delta(t-3) is zero everywhere except at the single instant t=3t = 3.
  3. Evaluate f(a)f(a) at a=3a = 3 and substitute a=3a = 3 into the exponential factor e−ase^{-as} to write the final transform.

Answer: 9e−3s9e^{-3s}

Watch out. At the bottom of the work for Problem 1, a stray note writes 23=t2^3 = t instead of evaluating f(3)=32=9f(3) = 3^2 = 9; always substitute t=at = a directly into f(t)=t2f(t) = t^2.

More problems

Problem (a): Hyperbolic cosine with a delayed impulse

Given: The impulse expression cosh⁡t δ(t−4)\cosh t \, \delta(t-4). Find: Its Laplace transform L[cosh⁡t δ(t−4)]\mathcal{L}[\cosh t \, \delta(t-4)].

  1. Match L[cosh⁡t δ(t−4)]\mathcal{L}[\cosh t \, \delta(t-4)] to the standard form L[f(t)δ(t−a)]\mathcal{L}[f(t)\delta(t-a)] with f(t)=cosh⁡tf(t) = \cosh t and delay a=4a = 4.
  2. Evaluate the function at the impulse instant a=4a = 4 to get the constant f(4)=cosh⁡4f(4) = \cosh 4.
  3. Substitute a=4a = 4 and f(4)=cosh⁡4f(4) = \cosh 4 into the impulse transform formula e−asf(a)e^{-as}f(a).

Answer: e−4scosh⁡4e^{-4s}\cosh 4

Problem 2: Sum of two impulse terms

Given: The combined impulse expression e−Atδ(t−2)+log⁡t δ(t−2)e^{-At}\delta(t-2) + \log t \, \delta(t-2). Find: Its Laplace transform L[e−Atδ(t−2)+log⁡t δ(t−2)]\mathcal{L}[e^{-At}\delta(t-2) + \log t \, \delta(t-2)].

  1. Split the transform across the sum into L[e−Atδ(t−2)]+L[log⁡t δ(t−2)]\mathcal{L}[e^{-At}\delta(t-2)] + \mathcal{L}[\log t \, \delta(t-2)] by linearity.
  2. Identify a=2a = 2 for both terms, with f1(t)=e−Atf_1(t) = e^{-At} in the first term and f2(t)=log⁡tf_2(t) = \log t in the second.
  3. Apply L[f(t)δ(t−a)]=e−asf(a)\mathcal{L}[f(t)\delta(t-a)] = e^{-as}f(a) to each piece by evaluating the functions at t=2t = 2.

Answer: e−2s(e−2A+log⁡2)e^{-2s}(e^{-2A} + \log 2)

Problem 3: Exponential switched by a delayed unit step

Given: The step-switched function e−3tu(t−1)e^{-3t}u(t-1). Find: Its Laplace transform L[e−3tu(t−1)]\mathcal{L}[e^{-3t}u(t-1)].

  1. Rewrite tt as (t−1+1)(t - 1 + 1) in the exponent so the time variable matches the shifted step u(t−1)u(t-1).
  2. Expand the exponent to e−3(t−1)−3u(t−1)e^{-3(t-1)-3}u(t-1) and factor out the constant e−3e^{-3} in front of the Laplace operator.
  3. Match the remaining L[e−3(t−1)u(t−1)]\mathcal{L}[e^{-3(t-1)}u(t-1)] to L[f(t−a)u(t−a)]\mathcal{L}[f(t-a)u(t-a)] with a=1a = 1 and unshifted function f(t)=e−3tf(t) = e^{-3t}.
  4. Take the transform of f(t)=e−3tf(t) = e^{-3t} to obtain fˉ(s)=1s+3\bar{f}(s) = \frac{1}{s+3}.
  5. Apply the second shifting theorem e−3⋅e−asfˉ(s)e^{-3} \cdot e^{-as}\bar{f}(s) with a=1a = 1 and combine the exponents.

Watch out. Do not apply the second shifting theorem directly to e−3tu(t−1)e^{-3t}u(t-1) as e−s1s+3e^{-s}\frac{1}{s+3}; you must first shift tt to (t−1)(t-1) inside the exponential, which pulls out the extra factor e−3e^{-3}.

Answer: e−3−ss+3\frac{e^{-3-s}}{s+3}