Laplace transform

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In the branch of mathematics called functional analysis, the Laplace transform, $scriptstylemathcal\{L\}\; left\{f(t)right\}$, is a linear operator on a function f(t) (original) with a real argument t (t ≥ 0) that transforms it to a function F(s) (image) with a complex argument s. This transformation is essentially bijective for the majority of practical uses; the respective pairs of f(t) and F(s) are matched in tables. The Laplace transform has the useful property that many relationships and operations over the originals f(t) correspond to simpler relationships and operations over the images F(s). The Laplace transform has many important applications in mathematics, physics, optics, electrical engineering, control engineering, signal processing, and probability theory. In mathematics, it is used for solving differential and integral equations. In physics, it is used for analysis of linear time-invariant systems such as electrical circuits, harmonic oscillators, optical devices, and mechanical systems. In this analysis, the Laplace transform is often interpreted as a transformation from the time-domain, in which inputs and outputs are functions of time, to the frequency-domain, where the same inputs and outputs are functions of complex angular frequency, or radians per unit time. Given a simple mathematical or functional description of an input or output to a system, the Laplace transform provides an alternative functional description that often simplifies the process of analyzing the behavior of the system, or in synthesizing a new system based on a set of specifications.

The Laplace transform is named in honor of mathematician and astronomer Pierre-Simon Laplace, who used the transform in his work on probability theory.

Formal definition

The Laplace transform of a function f(t), defined for all real numbers t ≥ 0, is the function F(s), defined by:

$F(s)\; =\; mathcal\{L\}\; left\{f(t)right\}=int\_\{0^-\}^infty\; e^\{-st\}\; f(t)\; ,dt.$

The lower limit of 0⁻ is short notation to mean

$lim\_\{varepsilonto\; 0+\}int\_\{-varepsilon\}^infty$

and assures the inclusion of the entire Dirac delta function δ(t) at 0 if there is such an impulse in f(t) at 0.

The parameter s is in general complex:

$s\; =\; sigma\; +\; i\; omega\; ,$

This integral transform has a number of properties that make it useful for analyzing linear dynamic systems. The most significant advantage is that differentiation and integration become multiplication and division, respectively, by s. (This is similar to the way that logarithms change an operation of multiplication of numbers to addition of their logarithms.) This changes integral equations and differential equations to polynomial equations, which are much easier to solve. Once solved, use of the inverse Laplace transform reverts back to the time domain.

Bilateral Laplace transform

When one says "the Laplace transform" without qualification, the unilateral or one-sided transform is normally intended. The Laplace transform can be alternatively defined as the bilateral Laplace transform or two-sided Laplace transform by extending the limits of integration to be the entire real axis. If that is done the common unilateral transform simply becomes a special case of the bilateral transform where the definition of the function being transformed is multiplied by the Heaviside step function.

The bilateral Laplace transform is defined as follows:

$F(s)\; =\; mathcal\{L\}left\{f(t)right\}\; =int\_\{-infty\}^\{+infty\}\; e^\{-st\}\; f(t),dt.$

Inverse Laplace transform

The inverse Laplace transform is given by the following complex integral, which is known by various names (the Bromwich integral, the Fourier-Mellin integral, and Mellin's inverse formula):

$f(t)\; =\; mathcal\{L\}^\{-1\}\; \{F(s)\}\; =\; frac\{1\}\{2\; pi\; i\}\; int\_\{\; gamma\; -\; i\; cdot\; infty\}^\{\; gamma\; +\; i\; cdot\; infty\}\; e^\{st\}\; F(s),ds,$

where $gamma$ is a real number so that the contour path of integration is in the region of convergence of F(s) normally requiring $gamma$ > Re(s_p) for every singularity s_p of F(s) and i² = −1. If all singularities are in the left half-plane, that is Re(s_p) < 0 for every s_p, then $gamma$ can be set to zero and the above inverse integral formula above becomes identical to the inverse Fourier transform.

An alternative formula for the inverse Laplace transform is given by Post's inversion formula.

Region of convergence

The Laplace transform F(s) typically exists for all complex numbers such that Re{s} > a, where a is a real constant which depends on the growth behavior of f(t), whereas the two-sided transform is defined in a range a < Re{s} < b. The subset of values of s for which the Laplace transform exists is called the region of convergence (ROC) or the domain of convergence. In the two-sided case, it is sometimes called the strip of convergence.

The integral defining the Laplace transform of a function may fail to exist for various reasons. For example, when the function has infinite discontinuities in the interval of integration, or when it increases so rapidly that exp(-pt) cannot dampen it sufficiently for convergence on the interval to take place. There are no specific conditions that one can check a function against to know in all cases if its Laplace transform can be taken, other than to say the defining integral converges. It is however easy to give theorems on cases where it may or may not be taken.

Properties and theorems

Given the functions f(t) and g(t), and their respective Laplace transforms F(s) and G(s):

$f(t)\; =\; mathcal\{L\}^\{-1\}\; \{\; F(s)\; \}$

$g(t)\; =\; mathcal\{L\}^\{-1\}\; \{\; G(s)\; \}$

the following table is a list of properties of unilateral Laplace transform:

!

	! Time domain

! Frequency domain

	! Comment

! Linearity

| $a\; f(t)\; +\; b\; g(t)$ | $a\; F(s)\; +\; b\; G(s)$ | Can be proved using basic rules of integration.

! Frequency differentiation

| $t\; f(t)$ | $-F\text{'}(s)$ |

! Frequency differentiation

| $t^\{n\}\; f(t)$ | $(-1)^\{n\}\; F^\{(n)\}(s)$ | More general form

! Differentiation

| $f\text{'}(t)$ | $s\; F(s)\; -\; f(0^-)$ | Write the exact integral form of the given function, and add another integral to complement the former to deduce the sum to indefinite integration of a differential. Next few steps are simple.

! Second Differentiation

| $f\text{'}\text{'}(t)$ | $s^2\; F(s)\; -\; s\; f(0^-)\; -\; f\text{'}(0^-)$ | Apply the Differentiation property to $f\text{'}(t)$.

! General Differentiation

| $f^\{(n)\}(t)$ | $s^n\; F(s)\; -\; s^\{n\; -\; 1\}\; f(0^-)\; -\; cdots\; -\; f^\{(n\; -\; 1)\}(0^-)$ | Follow the process briefed for the Second Differentiation.

! Frequency integration

| $frac\{f(t)\}\{t\}$ | $int\_s^infty\; F(sigma),\; dsigma$ |

! Integration

| $int\_0^t\; f(tau),\; dtau\; =\; u(t)\; *\; f(t)$ | $\{1\; over\; s\}\; F(s)$ | $u(t)$ is the Heaviside step function.

! Scaling

| $f(at)$ | $\{1\; over\; |a$

Properties of the unilateral Laplace transform

F left ({s over a} right ) |

! Frequency shifting

| $e^\{at\}\; f(t)$ | $F(s\; -\; a)$ |

! Time shifting

| $f(t\; -\; a)\; u(t\; -\; a)$ | $e^\{-as\}\; F(s)$ | $u(t)$ is the Heaviside step function

! Convolution

| $(f\; *\; g)(t)$ | $F(s)\; cdot\; G(s)$ |

! Periodic Function

| $f(t)$ | $\{1\; over\; 1\; -\; e^\{-Ts\}\}\; int\_0^T\; e^\{-st\}\; f(t),dt$ | $f(t)$ is a periodic function of period $T$ so that $f(t)\; =\; f(t\; +\; T),\; ;\; forall\; t$

• Initial value theorem:

$f(0^+)=lim\_\{sto\; infty\}\{sF(s)\}$

• Final value theorem:

$f(infty)=lim\_\{sto\; 0\}\{sF(s)\}$, all poles in left-hand plane.

The final value theorem is useful because it gives the long-term behaviour without having to perform partial fraction decompositions or other difficult algebra. If a function's poles are in the right hand plane (e.g. $e^t$ or $sin(t)$) the behaviour of this formula is undefined.

Proof of the Laplace transform of a function's derivative

It is often convenient to use the differentiation property of the Laplace transform to find the transform of a function's derivative. This can be derived from the basic expression for a Laplace transform as follows:

$mathcal\{L\}\; left\{f(t)right\}\; =int\_\{0^-\}^\{+infty\}\; e^\{-st\}\; f(t),dt$

$~~\; =\; left[frac\{f(t)e^\{-st\}\}\{-s\}\; right]\_\{0^-\}^\{+infty\}\; -$

int_{0^-}^{+infty} frac{e^{-st}}{-s} f'(t)dt (by parts)

$~~\; =\; left[-frac\{f(0)\}\{-s\}right]\; +$

frac{1}{s}mathcal{L}left{f'(t)right},

yielding

$mathcal\{L\}left\{frac\{df\}\{dt\}right\}\; =\; scdotmathcal\{L\}\; left\{\; f(t)\; right\}-f(0),$

and in the bilateral case, we have

$mathcal\{L\}left\{\; \{\; df\; over\; dt\; \}\; right\}$

= s int_{-infty}^{+infty} e^{-st} f(t),dt = s cdot mathcal{L} { f(t) }.

Relationship to other transforms

Fourier transform

The continuous Fourier transform is equivalent to evaluating the bilateral Laplace transform with complex argument s = iω or s = 2πfi:

$$

begin{array}{rcl} F(omega) & = & mathcal{F}left{f(t)right} [1em] & = & mathcal{L}left{f(t)right}|_{s = i omega} = F(s)|_{s = i omega}[1em] & = & int_{-infty}^{+infty} e^{-imath omega t} f(t),mathrm{d}t. end{array}

Note that this expression excludes the scaling factor $frac\{1\}\{sqrt\{2\; pi\}\}$, which is often included in definitions of the Fourier transform.

This relationship between the Laplace and Fourier transforms is often used to determine the frequency spectrum of a signal or dynamic system.

Mellin transform

The Mellin transform and its inverse are related to the two-sided Laplace transform by a simple change of variables. If in the Mellin transform

$G(s)\; =\; mathcal\{M\}left\{g(theta)right\}\; =\; int\_0^infty\; theta^s\; g(theta)\; frac\{dtheta\}\{theta\}$

we set θ = e^-t we get a two-sided Laplace transform.

Z-transform

The Z-transform is simply the Laplace transform of an ideally sampled signal with the substitution of

$z\; stackrel\{mathrm\{def\}\}\{=\}\; e^\{s\; T\}$

where $T\; =\; 1/f\_s$ is the sampling period (in units of time e.g., seconds) and $f\_s$ is the sampling rate (in samples per second or hertz)

Let

$Delta\_T(t)\; stackrel\{mathrm\{def\}\}\{=\}\; sum\_\{n=0\}^\{infty\}\; delta(t\; -\; n\; T)$

be a sampling impulse train (also called a Dirac comb) and

$x\_q(t)\; stackrel\{mathrm\{def\}\}\{=\}\; x(t)\; Delta\_T(t)\; =\; x(t)\; sum\_\{n=0\}^\{infty\}\; delta(t\; -\; n\; T)$

$=\; sum\_\{n=0\}^\{infty\}\; x(n\; T)\; delta(t\; -\; n\; T)\; =\; sum\_\{n=0\}^\{infty\}\; x[n]\; delta(t\; -\; n\; T)$

be the continuous-time representation of the sampled $x(t)$.

$x[n]\; stackrel\{mathrm\{def\}\}\{=\}\; x(nT)$ are the discrete samples of $x(t)$.

The Laplace transform of the sampled signal $x\_q(t)$ is

$X\_q(s)\; =\; int\_\{0^-\}^\{infty\}\; x\_q(t)\; e^\{-s\; t\}\; ,dt$

$=\; int\_\{0^-\}^\{infty\}\; sum\_\{n=0\}^\{infty\}\; x[n]\; delta(t\; -\; n\; T)\; e^\{-s\; t\}\; ,\; dt$

$=\; sum\_\{n=0\}^\{infty\}\; x[n]\; int\_\{0^-\}^\{infty\}\; delta(t\; -\; n\; T)\; e^\{-s\; t\}\; ,\; dt$

$=\; sum\_\{n=0\}^\{infty\}\; x[n]\; e^\{-n\; s\; T\}.$

This is precisely the definition of the Z-transform of the discrete function $x[n]$

$X(z)\; =\; sum\_\{n=0\}^\{infty\}\; x[n]\; z^\{-n\}$

with the substitution of $z\; leftarrow\; e^\{s\; T\}$.

Comparing the last two equations, we find the relationship between the Z-transform and the Laplace transform of the sampled signal:

$X\_q(s)\; =\; X(z)\; Big|\_\{z=e^\{sT\}\}.$

Borel transform

The integral form of the Borel transform is identical to the Laplace transform; indeed, these are sometimes mistakenly assumed to be synonyms. The generalized Borel transform generalizes the Laplace transform for functions not of exponential type.

Fundamental relationships

Since an ordinary Laplace transform can be written as a special case of a two-sided transform, and since the two-sided transform can be written as the sum of two one-sided transforms, the theory of the Laplace-, Fourier-, Mellin-, and Z-transforms are at bottom the same subject. However, a different point of view and different characteristic problems are associated with each of these four major integral transforms.

Table of selected Laplace transforms

The following table provides Laplace transforms for many common functions of a single variable. For definitions and explanations, see the Explanatory Notes at the end of the table.

Because the Laplace transform is a linear operator:

• The Laplace transform of a sum is the sum of Laplace transforms of each term.

$mathcal\{L\}left\{f(t)\; +\; g(t)\; right\}\; =\; mathcal\{L\}left\{f(t)right\}\; +\; mathcal\{L\}left\{\; g(t)\; right\}$

• The Laplace transform of a multiple of a function, is that multiple times the Laplace transformation of that function.

$mathcal\{L\}left\{a\; f(t)right\}\; =\; a\; mathcal\{L\}left\{\; f(t)right\}$

The unilateral Laplace transform is only valid when t is non-negative, which is why all of the time domain functions in the table below are multiples of the Heaviside step function, u(t).

ID	Function	Time domain $x(t)\; =\; mathcal\{L\}^\{-1\}\; left\{\; X(s)\; right\}$	Frequency domain $X(s)\; =\; mathcal\{L\}left\{\; x(t)\; right\}$	Region of convergence for causal systems
1	ideal delay	$delta(t-tau)$	$e^\{-tau\; s\}$
1a	unit impulse	$delta(t)$	$1$	$mathrm\{all\}\; s\; ,$
2	delayed nth power with frequency shift	$frac\{(t-tau)^n\}\{n!\}\; e^\{-alpha\; (t-tau)\}\; cdot\; u(t-tau)$	$frac\{e^\{-tau\; s\}\}\{(s+alpha)^\{n+1\}\}$	$s\; >\; 0\; ,$
2a	nth power (for integer n )	$\{\; t^n\; over\; n!\; \}\; cdot\; u(t)$	$\{\; 1\; over\; s^\{n+1\}\; \}$	$s\; >\; 0\; ,$
2a.1	qth power (for real q )	$\{\; t^q\; over\; Gamma(q+1)\; \}\; cdot\; u(t)$	$\{\; 1\; over\; s^\{q+1\}\; \}$	$s\; >\; 0\; ,$
2a.2	unit step	$u(t)$	$\{\; 1\; over\; s\; \}$	$s\; >\; 0\; ,$
2b	delayed unit step	$u(t-tau)$	$\{\; e^\{-tau\; s\}\; over\; s\; \}$	$s\; >\; 0\; ,$
2c	ramp	$t\; cdot\; u(t)$	$frac\{1\}\{s^2\}$	$s\; >\; 0\; ,$
2d	nth power with frequency shift	$frac\{t^\{n\}\}\{n!\}e^\{-alpha\; t\}\; cdot\; u(t)$	$frac\{1\}\{(s+alpha)^\{n+1\}\}$	$s\; >\; -\; alpha\; ,$
2d.1	exponential decay	$e^\{-alpha\; t\}\; cdot\; u(t)$	$\{\; 1\; over\; s+alpha\; \}$	$s\; >\; -\; alpha$
3	exponential approach	$(1-e^\{-alpha\; t\})\; cdot\; u(t)$	$frac\{alpha\}\{s(s+alpha)\}$	$s\; >\; 0$
4	sine	$sin(omega\; t)\; cdot\; u(t)$	$\{\; omega\; over\; s^2\; +\; omega^2\; \}$	$s\; >\; 0$
5	cosine	$cos(omega\; t)\; cdot\; u(t)$	$\{\; s\; over\; s^2\; +\; omega^2\; \}$	$s\; >\; 0$
6	hyperbolic sine	$sinh(alpha\; t)\; cdot\; u(t)$	$\{\; alpha\; over\; s^2\; -\; alpha^2\; \}$	s > > alpha |
7	hyperbolic cosine	$cosh(alpha\; t)\; cdot\; u(t)$	$\{\; s\; over\; s^2\; -\; alpha^2\; \}$	s > > alpha |
8	Exponentially-decaying sine wave	$e^\{alpha\; t\}\; sin(omega\; t)\; cdot\; u(t)$	$\{\; omega\; over\; (s-alpha\; )^2\; +\; omega^2\; \}$	$s\; >\; alpha$
9	Exponentially-decaying cosine wave	$e^\{alpha\; t\}\; cos(omega\; t)\; cdot\; u(t)$	$\{\; s-alpha\; over\; (s-alpha\; )^2\; +\; omega^2\; \}$	$s\; >\; alpha$
10	nth root	$sqrt[n]\{t\}\; cdot\; u(t)$	$s^\{-(n+1)/n\}\; cdot\; Gammaleft(1+frac\{1\}\{n\}right)$	$s\; >\; 0\; ,$
11	natural logarithm	$ln\; left\; (\; \{\; t\; over\; t\_0\; \}\; right\; )\; cdot\; u(t)$	$-\; \{\; t\_0\; over\; s\}\; [\; ln(t\_0\; s)+gamma\; ]$	$s\; >\; 0\; ,$
12	Bessel function of the first kind, of order n	$J\_n(omega\; t)\; cdot\; u(t)$	$frac\{\; omega^n\; left(s+sqrt\{s^2+\; omega^2\}right)^\{-n\}\}\{sqrt\{s^2\; +\; omega^2\}\}$	$s\; >\; 0\; ,$ $(n\; >\; -1)\; ,$
13	Modified Bessel function of the first kind, of order n	$I\_n(omega\; t)\; cdot\; u(t)$	$frac\{\; omega^n\; left(s+sqrt\{s^2-omega^2\}right)^\{-n\}\}\{sqrt\{s^2-omega^2\}\}$	s > > omega | ,
14	Bessel function of the second kind, of order 0	$Y\_0(alpha\; t)\; cdot\; u(t)$	$-\{2\; sinh^\{-1\}(s/alpha)\; over\; pi\; sqrt\{s^2+alpha^2\}\}$	$s\; >\; 0\; ,$
15	Modified Bessel function of the second kind, of order 0	$K\_0(alpha\; t)\; cdot\; u(t)$
16	Error function	$mathrm\{erf\}(t)\; cdot\; u(t)$	$\{e^\{s^2/4\}\; left(1\; -\; operatorname\{erf\}\; left(s/2right)right)\; over\; s\}$	$s\; >\; 0\; ,$
Explanatory notes: $u(t)\; ,$ represents the Heaviside step function. $delta(t)\; ,$ represents the Dirac delta function. $Gamma\; (z)\; ,$ represents the Gamma function. $gamma\; ,$ is the Euler-Mascheroni constant. $t\; ,$, a real number, typically represents time, although it can represent any independent dimension. $s\; ,$ is the complex angular frequency. $alpha\; ,$, $beta\; ,$, $tau\; ,$, and $omega\; ,$ are real numbers. $n\; ,$, is an integer. A causal system is a system where the impulse response h(t) is zero for all time t prior to t = 0. In general, the ROC for causal systems is not the same as the ROC for anticausal systems. See also causality.

s-Domain equivalent circuits and impedances

The Laplace transform is often used in circuit analysis, and simple conversions to the s-Domain of circuit elements can be made. Circuit elements can be transformed into impedances, very similar to phasor impedances.

Here is a summary of equivalents: : Note that the resistor is exactly the same in the time domain and the s-Domain. The sources are put in if there are initial conditions on the circuit elements. For example, if a capacitor has an initial voltage across it, or if the inductor has an initial current through it, the sources inserted in the s-Domain account for that.

The equivalents for current and voltage sources are simply derived from the transformations in the table above.

Examples: How to apply the properties and theorems

The Laplace transform is used frequently in engineering and physics; the output of a linear dynamic system can be calculated by convolving its unit impulse response with the input signal. Performing this calculation in Laplace space turns the convolution into a multiplication; the latter being easier to solve because of its algebraic form. For more information, see control theory.

The Laplace transform can also be used to solve differential equations and is used extensively in electrical engineering. The method of using the Laplace Transform to solve differential equations was developed by the English electrical engineer Oliver Heaviside.

The following examples, derived from applications in physics and engineering, will use SI units of measure. SI is based on meters for distance, kilograms for mass, seconds for time, and amperes for electric current.

Example #1: Solving a differential equation

The following example is based on concepts from nuclear physics.

Consider the following first-order, linear differential equation:

$frac\{dN\}\{dt\}\; =\; -lambda\; N.$

This equation is the fundamental relationship describing radioactive decay, where

$N\; =\; N(t)$

represents the number of undecayed atoms remaining in a sample of a radioactive isotope at time t (in seconds), and $lambda$ is the decay constant.

We can use the Laplace transform to solve this equation.

Rearranging the equation to one side, we have

$frac\{dN\}\{dt\}\; +\; lambda\; N\; =\; 0.$

Next, we take the Laplace transform of both sides of the equation:

$left(s\; tilde\{N\}(s)\; -\; N\_o\; right)\; +\; lambda\; tilde\{N\}(s)\; =\; 0$

where

$tilde\{N\}(s)\; =\; mathcal\{L\}\{N(t)\}$

and

$N\_o\; =\; N(0).$

Solving, we find

$tilde\{N\}(s)\; =\; \{\; N\_o\; over\; s\; +\; lambda\; \}.$

Finally, we take the inverse Laplace transform to find the general solution

$N(t)\; =\; mathcal\{L\}^\{-1\}\; \{tilde\{N\}(s)\}\; =\; mathcal\{L\}^\{-1\}\; left\{\; frac\{N\_o\}\{s\; +\; lambda\}\; right\}$

$=\; N\_o\; e^\{-lambda\; t\},$

which is indeed the correct form for radioactive decay.

Example #2: Deriving the complex impedance for a capacitor

This example is based on the principles of electrical circuit theory.

The constitutive relation governing the dynamic behavior of a capacitor is the following differential equation:

$i\; =\; C\; \{\; dv\; over\; dt\}$

where C is the capacitance (in farads) of the capacitor, i = i(t) is the electrical current (in amperes) flowing through the capacitor as a function of time, and v = v(t) is the voltage (in volts) across the terminals of the capacitor, also as a function of time.

Taking the Laplace transform of this equation, we obtain

$I(s)\; =\; C\; left(s\; V(s)\; -\; V\_o\; right)$

where

$I(s)\; =\; mathcal\{L\}\; \{\; i(t)\; \},$

$V(s)\; =\; mathcal\{L\}\; \{\; v(t)\; \},$ and

$V\_o\; =\; v(t)|\_\{t=0\}.$

Solving for V(s) we have

$V(s)\; =\; \{\; I(s)\; over\; sC\; \}\; +\; \{\; V\_o\; over\; s\; \}.$

The definition of the complex impedance Z (in ohms) is the ratio of the complex voltage V divided by the complex current I while holding the initial state V_o at zero:

$Z(s)\; =\; \{\; V(s)\; over\; I(s)\; \}\; bigg|\_\{V\_o\; =\; 0\}.$

Using this definition and the previous equation, we find:

$Z(s)\; =\; frac\{1\}\{sC\},$

which is the correct expression for the complex impedance of a capacitor.

Example #3: Finding the transfer function from the impulse response

This example is based on concepts from signal processing, and describes the dynamic behavior of a damped harmonic oscillator. See also RLC circuit.

Consider a linear time-invariant system with impulse response

$h(t)\; =\; A\; e^\{-\; alpha\; t\}\; cos(omega\_d\; t\; -\; phi\_d)\; ,$

such that

$omega\_d\; t\; -\; phi\_d\; ge\; 0\; ,$

where t is the time (in seconds), and

$0\; le\; phi\_d\; le\; 2\; pi$

is the phase delay (in radians).

Suppose that we want to find the transfer function of the system. We begin by noting that

$h(t)\; =\; A\; e^\{-\; alpha\; t\}\; cos\; left[omega\_d\; (t\; -\; t\_d)\; right]\; cdot\; u(t\; -\; t\_d)\; ,$

where

$t\_d\; =\; \{\; phi\_d\; over\; omega\_d\; \}$

is the time delay of the system (in seconds), and $u(t)$ is the Heaviside step function.

The transfer function is simply the Laplace transform of the impulse response:

$H(s)\; =\; mathcal\{L\}\; \{\; h(t)\; \}\; =\; A\; e^\{-s\; t\_d\}\; \{(s\; +\; alpha)\; over\; (s\; +\; alpha)^2\; +\; omega\_d^2\; \}$

$=\; A\; e^\{-s\; t\_d\}\; \{(s\; +\; alpha)\; over\; (s^2\; +\; 2\; alpha\; s\; +\; alpha^2)\; +\; omega\_d^2\; \}$

$=\; A\; e^\{-s\; t\_d\}\; \{(s\; +\; alpha)\; over\; (s^2\; +\; 2\; alpha\; s\; +\; omega\_0^2\; )\; \}$

where

$omega\_0\; =\; sqrt\{alpha^2\; +\; omega\_d^2\}$

is the (undamped) natural frequency or resonance of the system (in radians per second).

Example #4: Method of partial fraction expansion

Consider a linear time-invariant system with transfer function

$H(s)\; =\; frac\{1\}\{(s+alpha)(s+beta)\}.$

The impulse response is simply the inverse Laplace transform of this transfer function:

$h(t)\; =\; mathcal\{L\}^\{-1\}\{H(s)\}.$

To evaluate this inverse transform, we begin by expanding H(s) using the method of partial fraction expansion:

$H(s)\; =\; frac\{1\}\{(s+alpha)(s+beta)\}\; =\; \{\; P\; over\; (s+alpha)\; \}\; +\; \{\; R\; over\; (s+beta)\; \}$

for unknown constants P and R. To find these constants, we evaluate

$P\; =\; left.\{1\; over\; (s+beta)\}right|\_\{s=-alpha\}\; =\; \{1\; over\; (beta\; -\; alpha)\}$

and

$R\; =\; left.\{1\; over\; (s+alpha)\}right|\_\{s=-beta\}\; =\; \{1\; over\; (alpha\; -\; beta)\}\; =\; \{-1\; over\; (beta\; -\; alpha)\}\; =\; -\; P\; .$

Substituting these values into the expression for H(s), we find

$H(s)\; =\; left(frac\{1\}\{beta-alpha\}\; right)\; cdot\; left(\; \{\; 1\; over\; (s+alpha)\; \}\; -\; \{\; 1\; over\; (s+beta)\; \}\; right).$

Finally, using the linearity property and the known transform for exponential decay (see Item #3 in the Table of Laplace Transforms, above), we can take the inverse Laplace transform of H(s) to obtain:

$h(t)\; =\; mathcal\{L\}^\{-1\}\{H(s)\}\; =\; frac\{1\}\{beta-alpha\}left(e^\{-alpha\; t\}-e^\{-beta\; t\}right),$

which is the impulse response of the system.

Example #5: Mixing sines, cosines, and exponentials

Time function	Laplace transform
$e^\{-alpha\; t\}left[cos\{(omega\; t)\}+left(frac\{beta-alpha\}\{omega\}right)sin\{(omega\; t)\}right]u(t)$	$frac\{s+beta\}\{(s+alpha)^2+omega^2\}$

Starting with the Laplace transform

$X(s)\; =\; frac\{s+beta\}\{(s+alpha)^2+omega^2\},$

we find the inverse transform by first adding and subtracting the same constant α to the numerator:

$X(s)\; =\; frac\{s+alpha\; \}\; \{\; (s+alpha)^2+omega^2\}\; +\; frac\{beta\; -\; alpha\; \}\{(s+alpha)^2+omega^2\}.$

By the shift-in-frequency property, we have

$x(t)\; =\; e^\{-alpha\; t\}\; mathcal\{L\}^\{-1\}\; left\{\; \{s\; over\; s^2\; +\; omega^2\}\; +\; \{\; beta\; -\; alpha\; over\; s^2\; +\; omega^2\; \}\; right\}$

$=\; e^\{-alpha\; t\}\; mathcal\{L\}^\{-1\}\; left\{\; \{s\; over\; s^2\; +\; omega^2\}\; +\; left(\{\; beta\; -\; alpha\; over\; omega\; \}\; right)\; left(\{\; omega\; over\; s^2\; +\; omega^2\; \}\; right)\; right\}$

$=\; e^\{-alpha\; t\}\; left[\; mathcal\{L\}^\{-1\}\; left\{\; \{s\; over\; s^2\; +\; omega^2\}\; right\}\; +\; left(\{\; beta\; -\; alpha\; over\; omega\; \}\; right)\; mathcal\{L\}^\{-1\}\; left\{\; \{\; omega\; over\; s^2\; +\; omega^2\; \}\; right\}\; right].$

Finally, using the Laplace transforms for sine and cosine (see the table, above), we have

$x(t)\; =\; e^\{-alpha\; t\}\; left[cos\{(omega\; t)\}u(t)+left(frac\{beta-alpha\}\{omega\}right)sin\{(omega\; t)\}u(t)right].$

$x(t)\; =\; e^\{-alpha\; t\}\; left[cos\{(omega\; t)\}+left(frac\{beta-alpha\}\{omega\}right)sin\{(omega\; t)\}right]u(t).$

Example #6: Phase delay

Time function	Laplace transform
$sin\{(omega\; t+phi)\}$	$frac\{ssinphi+omega\; cosphi\}\{s^2+omega^2\}$
$cos\{(omega\; t+phi)\}$	$frac\{scosphi\; -\; omega\; sinphi\}\{s^2+omega^2\}$

Starting with the Laplace transform,

$X(s)\; =\; frac\{ssinphi+omega\; cosphi\}\{s^2+omega^2\}$

we find the inverse by first rearranging terms in the fraction:

$X(s)\; ,!$	$\{\}\; =\; frac\{s\; sin\; phi\}\{s^2\; +\; omega^2\}\; +\; frac\{omega\; cos\; phi\}\{s^2\; +\; omega^2\}$
	$\{\}\; =\; (sin\; phi)\; left(frac\{s\}\{s^2\; +\; omega^2\}\; right)\; +\; (cos\; phi)\; left(frac\{omega\}\{s^2\; +\; omega^2\}\; right).$

We are now able to take the inverse Laplace transform of our terms:

$x(t)\; ,!$	$\{\}\; =\; (sin\; phi)\; mathcal\{L\}^\{-1\}left\{frac\{s\}\{s^2\; +\; omega^2\}\; right\}\; +\; (cos\; phi)\; mathcal\{L\}^\{-1\}left\{frac\{omega\}\{s^2\; +\; omega^2\}\; right\}$
	$\{\}=(sin\; phi)(cos\; omega\; t)\; +\; (sin\; omega\; t)(cos\; phi).\; ,!$

To simplify this answer, we must recall the trigonometric identity that

$a\; sin\; omega\; t\; +\; b\; cos\; omega\; t\; =\; sqrt\{a^2+b^2\}\; cdot\; sin\; left(omega\; t\; +\; arctan\; (b/a)\; right)$

and apply it to our value for x(t):

We can apply similar logic to find that

$mathcal\{L\}^\{-1\}\; left\{\; frac\{scosphi\; -\; omega\; sinphi\}\{s^2+omega^2\}\; right\}\; =\; cos\{(omega\; t+phi)\}.$

History

From 1744, Leonhard Euler investigated integrals of the form:

$z\; =\; int\; X(x)\; e^\{ax\}\; dx$ and $z\; =\; int\; X(x)\; x^A\; dx$,

— as solutions of differential equations but did not pursue the matter very far. Joseph Louis Lagrange was an admirer of Euler and, in his work on integrating probability density functions, investigated expressions of the form:

$int\; X(x)\; e^\{-\; a\; x\; \}\; a^x\; dx$

— which some modern historians have interpreted within modern Laplace transform theory.

These types of integrals seem first to have attracted Laplace's attention in 1782 where he was following in the spirit of Euler in using the integrals themselves as solutions of equations. However, in 1785, Laplace took the critical step forward when, rather than just look for a solution in the form of an integral, he started to apply the transforms in the sense that was later to become popular. He used an integral of the form:

$int\; x^s\; phi\; (s)\; dx$,

— akin to a Mellin transform, to transform the whole of a difference equation, in order to look for solutions of the transformed equation. He then went on to apply the Laplace transform in the same way and started to derive some of its properties, beginning to appreciate its potential power.

Laplace also recognised that Joseph Fourier's method of Fourier series for solving the diffusion equation could only apply to a limited region of space as the solutions were periodic. In 1809, Laplace applied the eponymous transform to find solutions that diffused indefinitely in space.

See also

• Pierre-Simon Laplace
• Fourier transform
• Analog signal processing
• Laplace transform applied to differential equations

References

Bibliography

Modern

• G.A. Korn and T.M. Korn, Mathematical Handbook for Scientists and Engineers, McGraw-Hill Companies; 2nd edition (June 1967). ISBN 0-0703-5370-0
• A. D. Polyanin and A. V. Manzhirov, Handbook of Integral Equations, CRC Press, Boca Raton, 1998. ISBN 0-8493-2876-4
• William McC. Siebert, Circuits, Signals, and Systems, MIT Press, Cambridge, Massachusetts, 1986. ISBN 0-262-19229-2
• Davies, Brian, Integral transforms and their applications, Third edition, Springer, New York, 2002. ISBN 0-387-95314-0
• Wolfgang Arendt, Charles J.K. Batty, Matthias Hieber, and Frank Neubrander. Vector-Valued Laplace Transforms and Cauchy Problems, Birkhäuser Basel, 2002. ISBN-10:3764365498

Historical

• Euler, L. (1744) "De constructione aequationum", Opera omnia 1st series, 22:150-161
• — (1753) "Methodus aequationes differentiales", Opera omnia 1st series, 22:181-213
• — (1769) Institutiones calculi integralis 2, Chs.3-5, in Opera omnia 1st series, 12
• Grattan-Guinness, I (1997) "Laplace's integral solutions to partial differential equations", in Gillispie, C. C. Pierre Simon Laplace 1749-1827: A Life in Exact Science, Princeton: Princeton University Press, ISBN 0-691-01185-0
• Lagrange, J. L. (1773) "Mémoire sur l'utilité de la méthode", Œuvres de Lagrange, 2:171-234

External links

• Online Computation of the transform or inverse transform, wims.unice.fr
• Tables of Integral Transforms at EqWorld: The World of Mathematical Equations.
• Laplace Transform Module by John H. Mathews
• Good explanations of the initial and final value theorems
• Laplace Transform Table at eFunda: Engineering Fundamentals.
• Laplace and Heaviside at Interactive maths.
• Laplace Transform Table and Examples at Vibrationdata.
• Laplace Transform Cookbook at Syscomp Electronic Design.

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$x(t)\; ,!$	$\{\}\; =\; sqrt\{cos^2\; phi\; +\; sin^2\; phi\}\; cdot\; sin\; left(omega\; t\; +\; arctan\; left(frac\{sin\; phi\}\{cos\; phi\}\; right)\; right)$
	$\{\}=\; sin\; (omega\; t\; +\; phi)\; .\; ,!$