Unit Step Function Laplace Transform

Heaviside steps, the second shifting theorem, and piecewise inputs written as u(t โˆ’ a)
Laplace transform of u(t - 3)
Laplace transform of f(t) = (t-2)^2 for t >= 2, 0 otherwise
Laplace transform of f(t) = 3 on [0,4) and 0 for t >= 4
Inverse Laplace transform of e^(-5s)/(s^2 + 1)

The Heaviside Step Function

The unit step (Heaviside) function switches on at t=at = a:

u(tโˆ’a)={0,t<a1,tโ‰ฅa(aโ‰ฅ0)u(t-a) = \begin{cases} 0, & t < a \\ 1, & t \ge a \end{cases} \qquad (a \ge 0)

Its transform follows straight from the definition, and the integral converges only for s>0s > 0:

L{u(tโˆ’a)}=โˆซ0โˆžeโˆ’stu(tโˆ’a)โ€‰dt=โˆซaโˆžeโˆ’stโ€‰dt=[โˆ’eโˆ’sts]aโˆž=eโˆ’ass\mathcal{L}\{u(t-a)\} = \int_0^{\infty} e^{-st}u(t-a)\,dt = \int_a^{\infty} e^{-st}\,dt = \left[\frac{-e^{-st}}{s}\right]_a^{\infty} = \frac{e^{-as}}{s}

Writing piecewise functions with steps is the whole point. A function that is 00, then turns on at aa and off at bb, is a window:

u(tโˆ’a)โˆ’u(tโˆ’b)u(t-a) - u(t-b)

So f(t)=3f(t) = 3 on [0,4)[0,4) and 00 afterwards becomes 3โˆ’3u(tโˆ’4)3 - 3u(t-4). Building this expression correctly is the step where most of the work โ€” and most of the errors โ€” live. The value assigned at the single point t=at = a never affects the transform.

The Second Shifting Theorem

If L{f(t)}=F(s)\mathcal{L}\{f(t)\} = F(s), then a delayed copy of ff transforms to

L{u(tโˆ’a)f(tโˆ’a)}=eโˆ’asF(s)\mathcal{L}\{u(t-a)f(t-a)\} = e^{-as}F(s)

Read the left side carefully: the function must be f(tโˆ’a)f(t-a), shifted by the same aa as the step. A factor of eโˆ’ase^{-as} in the ss-domain always means a time delay of aa.

When the function is not pre-shifted, use the equivalent form

L{u(tโˆ’a)g(t)}=eโˆ’asโ€‰L{g(t+a)}\mathcal{L}\{u(t-a)g(t)\} = e^{-as}\,\mathcal{L}\{g(t+a)\}

Inverting runs the same theorem backwards: Lโˆ’1{eโˆ’asF(s)}=u(tโˆ’a)f(tโˆ’a)\mathcal{L}^{-1}\{e^{-as}F(s)\} = u(t-a)f(t-a). For example Lโˆ’1{eโˆ’5ss2+1}=u(tโˆ’5)sinโก(tโˆ’5)\mathcal{L}^{-1}\left\{\dfrac{e^{-5s}}{s^2+1}\right\} = u(t-5)\sin(t-5).

Convolution handles a product of transforms: Lโˆ’1{F(s)G(s)}=(fโˆ—g)(t)=โˆซ0tf(ฯ„)g(tโˆ’ฯ„)โ€‰dฯ„\mathcal{L}^{-1}\{F(s)G(s)\} = (f*g)(t) = \int_0^t f(\tau)g(t-\tau)\,d\tau. This is why eโˆ’ase^{-as} times F(s)F(s) is a shift โ€” convolving with ฮด(tโˆ’a)\delta(t-a) translates ff.

All of this assumes ff is piecewise continuous and of exponential order, so the transform exists.

Common Mistakes to Avoid

  • Using f(t)f(t) where the theorem needs f(tโˆ’a)f(t-a). L{u(tโˆ’2)t2}โ‰ eโˆ’2sโ‹…2/s3\mathcal{L}\{u(t-2)t^2\} \neq e^{-2s}\cdot 2/s^3; you must first rewrite t2=(tโˆ’2)2+4(tโˆ’2)+4t^2 = (t-2)^2 + 4(t-2) + 4.
  • Getting the window backwards. "On during [a,b][a,b]" is u(tโˆ’a)โˆ’u(tโˆ’b)u(t-a) - u(t-b); reversing the order flips the sign of the whole pulse.
  • Forgetting s>0s > 0. The improper integral diverges otherwise, and the eโˆ’stโ†’0e^{-st} \to 0 step at the upper limit is only valid there.
  • Multiplying the shifts instead of adding. Each switch contributes its own additive term; steps do not compose by multiplication.
  • Confusing the two shifting theorems. eโˆ’asF(s)e^{-as}F(s) is a shift in tt; F(sโˆ’a)F(s-a) corresponds to eatf(t)e^{at}f(t), a shift in ss.
  • Reassembling an inverse without the u(tโˆ’a)u(t-a) factor, which would incorrectly switch the term on for all tt.

Examples

Step 1: By definition, L{u(tโˆ’3)}=โˆซ0โˆžeโˆ’stu(tโˆ’3)โ€‰dt\mathcal{L}\{u(t-3)\} = \displaystyle\int_0^{\infty} e^{-st}u(t-3)\,dt
Step 2: The step is 00 below t=3t = 3, so the lower limit becomes 33: โˆซ3โˆžeโˆ’stโ€‰dt\displaystyle\int_3^{\infty} e^{-st}\,dt
Step 3: =[โˆ’eโˆ’sts]3โˆž= \left[\dfrac{-e^{-st}}{s}\right]_3^{\infty}; for s>0s > 0 the upper limit gives 00
Step 4: =0โˆ’(โˆ’eโˆ’3ss)=eโˆ’3ss= 0 - \left(\dfrac{-e^{-3s}}{s}\right) = \dfrac{e^{-3s}}{s}
Answer: eโˆ’3ss\dfrac{e^{-3s}}{s}, valid for s>0s > 0

Step 1: Write it with a step: f(t)=u(tโˆ’2)(tโˆ’2)2f(t) = u(t-2)(t-2)^2
Step 2: This is already in the form u(tโˆ’a)g(tโˆ’a)u(t-a)g(t-a) with a=2a = 2 and g(t)=t2g(t) = t^2
Step 3: G(s)=L{t2}=2!s3=2s3G(s) = \mathcal{L}\{t^2\} = \dfrac{2!}{s^3} = \dfrac{2}{s^3}
Step 4: Second shifting theorem: multiply by eโˆ’as=eโˆ’2se^{-as} = e^{-2s}
Answer: 2eโˆ’2ss3\dfrac{2e^{-2s}}{s^3}

Step 1: As a window: f(t)=3[u(t)โˆ’u(tโˆ’4)]=3โˆ’3u(tโˆ’4)f(t) = 3\big[u(t) - u(t-4)\big] = 3 - 3u(t-4)
Step 2: L{3}=3s\mathcal{L}\{3\} = \dfrac{3}{s}
Step 3: L{3u(tโˆ’4)}=3โ‹…eโˆ’4ss\mathcal{L}\{3u(t-4)\} = 3 \cdot \dfrac{e^{-4s}}{s}
Step 4: Subtract by linearity: 3sโˆ’3eโˆ’4ss\dfrac{3}{s} - \dfrac{3e^{-4s}}{s}
Answer: 3(1โˆ’eโˆ’4s)s\dfrac{3\left(1 - e^{-4s}\right)}{s}

Frequently Asked Questions

L{u(t - a)} = e^(-as)/s for s > 0. With a = 0 this reduces to L{1} = 1/s, since u(t) is just the constant 1 on the domain of the transform.

It states that L{u(t-a) f(t-a)} = e^(-as) F(s). In words, delaying a signal by a in the time domain multiplies its transform by e^(-as). Reading it backwards inverts any transform containing an exponential factor.

Rewrite the function in powers of (t - a) first, or use the alternative form L{u(t-a) g(t)} = e^(-as) L{g(t + a)}. For example, u(t-2)t^2 needs t^2 expressed as (t-2)^2 + 4(t-2) + 4.

Convolution says the inverse of a product F(s)G(s) is the integral from 0 to t of f(tau)g(t-tau) d tau. Since e^(-as) is the transform of the shifted impulse, multiplying by it convolves f with delta(t - a), which simply translates f โ€” exactly the second shifting theorem.

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