The Inverse Laplace Transform Formula and Its Properties

The Bromwich integral that defines the inverse Laplace transform, plus the properties that make it usable: linearity, shifting, scaling and convolution.

The Inverse Laplace Transform Formula and Its Properties

The inverse Laplace transform formula is the Bromwich integral, a contour integral in the complex plane. Almost no engineer or student evaluates it directly. Instead, decompose F(s) into standard forms and apply a small set of properties: linearity, shifting, and convolution. That recovers f(t) without integrating. Here is the formal definition and the rules you will actually use.

The Bromwich Integral: The Formal Definition

The inverse Laplace transform is defined by the Bromwich integral (Churchill, Operational Mathematics, §6):

ℒ⁻¹{F(s)} = f(t) = (1 / (2πi)) ∫_{c-i∞}^{c+i∞} F(s) e^{st} ds for t ≥ 0

The integration runs along a vertical line Re(s) = c, where c lies to the right of all singularities of F(s). Use the Bromwich integral only when F(s) is non‑rational, for example, when it contains terms like e^{−as} or log(s). For rational F(s), the residue method (Churchill §7) converts the contour integral into a sum of residues at the poles of F(s). In practice, that is identical to performing a partial‑fraction decomposition and looking up the result.

Inverse Laplace Transform Properties You Actually Use

The four properties below, plus the convolution theorem, are the tools that let you invert rational F(s) without writing a contour integral. Each property is demonstrated with a one‑line example.

Linearity

ℒ⁻¹{αF(s) + βG(s)} = α f(t) + β g(t).

First Shifting Theorem

ℒ⁻¹{F(s−a)} = e^{at} f(t).

The shift in s multiplies the time‑domain result by e^{at}.

Second Shifting Theorem

ℒ⁻¹{e^{−as}F(s)} = u(t−a) f(t−a), where u(t−a) is the unit step function.

Example: ℒ⁻¹{e^{−2s}·1/(s+3)} = u(t−2) e^{-3(t−2)}.

Derivative in s

ℒ⁻¹{F'(s)} = −t f(t).

Convolution Theorem and Residue Method

The convolution theorem states ℒ⁻¹{F(s)G(s)} = (f * g)(t) = ∫₀ᵗ f(τ)g(t−τ) dτ. It is the fundamental reason the s‑domain product corresponds to a time‑domain convolution. For a full worked example, refer to the treatment of the convolution theorem in Boyce & DiPrima §6.6. For most practical inversions, use the residue method instead: the inverse of a rational F(s) is the sum of the residues of F(s)e^{st} at its poles. That is what partial‑fraction decomposition is doing algebraically. Churchill §7 gives the formal statement.

Inverse Laplace Transform Property Summary Table
Propertys‑Domain Formt‑Domain Result
LinearityαF(s) + βG(s)α f(t) + β g(t)
First Shifting TheoremF(s−a)e^{at} f(t)
Second Shifting Theoreme^{−as}F(s)u(t−a) f(t−a)
Derivative in sF'(s)−t f(t)
Convolution TheoremF(s)G(s)(f * g)(t)
Residue MethodF(s)e^{st} at polesSum of residues

Common Questions

When do I actually need to evaluate the Bromwich integral?

Only when F(s) is non‑rational, for example, if it contains e^{−as} or log(s). For rational functions, partial‑fraction decomposition and the residue method give the same result more quickly. Churchill's Operational Mathematics §7 covers the residue method as the practical alternative.

How do I invert a function with repeated poles?

Use the correct partial‑fraction form: for a pole at s = p of order m, include terms A₀/(s−p) + A₁/(s−p)² + … + A_{m−1}/(s−p)^{m}. The wrong form, using a single term with a quadratic denominator, will produce the wrong time‑domain result.

What is the difference between the first and second shifting theorems?

The first shifting theorem (frequency shift) multiplies f(t) by e^{at} when F(s) is shifted to F(s−a). The second shifting theorem (time shift) delays f(t) by a and multiplies by the unit step function u(t−a) when F(s) is multiplied by e^{−as}. They are not interchangeable.

Can I apply the final value theorem to any F(s)?

No. The final value theorem requires all poles of sF(s) to lie in the left half‑plane (Re(s) < 0). If F(s) has poles on the imaginary axis, for example, an undamped oscillator with poles at s = ±iω, the theorem gives a finite value when the true response oscillates indefinitely. This is a common failure mode.

How do I handle complex conjugate poles in partial fractions?

Keep the pair together. Instead of decomposing into two complex terms, use a quadratic denominator and a linear numerator: (As+B)/[(s−a)²+ω²]. Then match to the damped sine/cosine transform pairs (Kreyszig Table 6.9).

What do I do when the numerator degree equals the denominator degree?

Perform polynomial long division first.Skipping this step produces an algebraic error.

Which textbook has the most complete transform table?

Kreyszig Table 6.9 contains 23 transform pairs, which covers the majority of hand‑computation cases. For an exhaustive reference, Abramowitz & Stegun Chapter 29 lists 134 pairs. For classroom‑style worked problems, Boyce & DiPrima Chapter 6 exercises cover all common pole configurations.