Laplace transform
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In mathematics, the Laplace transform is a powerful technique for analyzing linear time-invariant systems such as electrical circuits, harmonic oscillators, optical devices, and mechanical systems, to name just a few. 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 an important concept from the branch of mathematics called functional analysis.
In actual physical systems the Laplace transform is often interpreted as a transformation from the time-domain point of view, in which inputs and outputs are understood as functions of time, to the frequency-domain point of view, where the same inputs and outputs are seen as functions of complex angular frequency, or radians per unit time. This transformation not only provides a fundamentally different way to understand the behavior of the system, but it also drastically reduces the complexity of the mathematical calculations required to analyze the system.
The Laplace transform has many important applications in physics, optics, electrical engineering, control engineering, signal processing, and probability theory.
The Laplace transform is named in honor of mathematician and astronomer Pierre-Simon Laplace, who used the transform in his work on probability theory. The transform was discovered originally by Leonhard Euler, the prolific eighteenth-century Swiss mathematician.
- 1 Formal definition
- 2 Region of convergence
- 3 Properties and theorems
- 3.1 Laplace transform of a function's derivative
- 3.2 Relationship to other transforms
- 3.2.1 Fourier transform
- 3.2.2 Mellin transform
- 3.2.3 Z-transform
- 3.2.4 Borel transform
- 3.2.5 Fundamental relationships
- 4 Table of selected Laplace transforms
- 5 s-Domain equivalent circuits and impedances
- 6 Examples: How to apply the properties and theorems
- 6.3 Example #1: Solving a differential equation
- 6.4 Example #2: Deriving the complex impedance for a capacitor
- 6.5 Example #3: Finding the transfer function from the impulse response
- 6.6 Example #4: Method of partial fraction expansion
- 6.7 Example #5: Mixing sines, cosines, and exponentials
- 6.8 Example #6: Phase delay
- 7 References
- 8 See also
- 9 External links
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 \left\ =\int_^\infty e^ f(t)\,dt.]
The parameter s is in general complex:
- [s = \sigma + i \omega. \, ]
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\left\ =\int_^ e^ f(t)\,dt.]
Inverse Laplace transform
The inverse Laplace transform is the Bromwich integral, which is a complex integral given by:
- [f(t) = \mathcal^ \ = \frac \int_^ e^ F(s)\,ds,]
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 > 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 < 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.
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^ \ ]
- [ g(t) = \mathcal^ \ ]
- Linearity
- [\mathcal\left\ = a F(s) + b G(s) ]
- Scaling
- Initial value theorem
- Final value theorem
- Frequency shifting
- Time shifting
- [n]th-power shifting
- Periodic Function period [T]
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. For the unilateral case, this approach becomes:
- [ \mathcal\left\ \right\} = s \int_^ e^ f(t)\,dt - f(0^-) = s \cdot \mathcal \ - f(0^-) ]
- [ \mathcal\left\ \right\} = s \int_^ e^ f(t)\,dt = s \cdot \mathcal \ ]
Relationship to other transforms
Fourier transform
The continuous Fourier transform is equivalent to evaluating the bilateral Laplace transform with complex argument [s = i\omega]:
- :[F(\omega) = \mathcal\left\ ]
- :::[= \mathcal\left\|_ = F(s)|_ ]
- :::[= \int_^ e^ f(t)\,\mathrmt.]
This relationship between the Laplace and Fourier transforms is often used to determine the frequency spectrum of a signal or dynamical 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\left\ = \int_0^\infty \theta^s g(\theta) \frac]
Z-transform
The Z-transform is simply the Laplace transform of an ideally sampled signal with the substitution of
- [ z \equiv e^ \ ]
- 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)
- [ \Delta_T(t) \equiv \sum_^ \delta(t - n T) ]
- [ x_q(t) \equiv x(t) \Delta_T(t) = x(t) \sum_^ \delta(t - n T) ]
- : [ = \sum_^ x(n T) \delta(t - n T) = \sum_^ x[n] \delta(t - n T) ]
- [ x[n] \equiv x(nT) \ ] are the discrete samples of [ x(t) \ ].
- [X_q(s) = \int_^ x_q(t) e^ \,dt ]
- :[ \ = \int_^ \sum_^ x[n] \delta(t - n T) e^ \, dt ]
- :[ \ = \sum_^ x[n] \int_^ \delta(t - n T) e^ \, dt ]
- :[ \ = \sum_^ x[n] e^.]
- [ X(z) = \sum_^ x[n] z^ ]
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|_}.]
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.
The Laplace transform of a sum is the sum of Laplace transforms of each term. The Laplace transform of a multiple of a function, is that multiple times the Laplace tranformation of that function. Laplace transforms are only valid when t is greater than [0^-], which is why everything in the table below is a multiple of u(t). Here is a list of common transforms:
| ID | Function | Time domain [x(t) = \mathcal^ \left\] | Laplace domain [X(s) = \mathcal\left\] | Region of convergence for causal systems | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | ideal delay | [ \delta(t-\tau) \ ] | [ e^ \ ] | |||||||||||
| 1a | unit impulse | [ \delta(t) \ ] | [ 1 \ ] | [ \mathrm \ s \,] | ||||||||||
| 2 | delayed nth power with frequency shift | [\frac e^ \cdot u(t-\tau) ] | [ \frac}} ] | [ s > 0 \, ] | ||||||||||
| 2a | nth power | [ \cdot u(t) ] | [ } ] | [ s > 0 \, ] | ||||||||||
| 2a.1 | qth power | [ \cdot u(t) ] | [ } ] | [ s > 0 \, ] | ||||||||||
| 2a.2 | unit step | [ u(t) \ ] | [ ] | [ s > 0 \, ] | ||||||||||
| 2b | delayed unit step | [ u(t-\tau) \ ] | [ \over s } ] | [ s > 0 \, ] | ||||||||||
| 2c | ramp | [ t \cdot u(t)\ ] | [\frac] | [ s > 0 \, ] | ||||||||||
| 2d | nth power with frequency shift | [\frac}e^ \cdot u(t) ] | [\frac}] | [ s > - \alpha \, ] | ||||||||||
| 2d.1 | exponential decay | [ e^ \cdot u(t) \ ] | [ ] | [ s > - \alpha \ ] | ||||||||||
| 3 | exponential approach | [( 1-e^) \cdot u(t) \ ] | [\frac ] | [ s > 0\ ] | ||||||||||
| 4 | sine | [ \sin(\omega t) \cdot u(t) \ ] | [ ] | [ s > 0 \ ] | ||||||||||
| 5 | cosine | [ \cos(\omega t) \cdot u(t) \ ] | [ ] | [ s > 0 \ ] | ||||||||||
| 6 | hyperbolic sine | [ \sinh(\alpha t) \cdot u(t) \ ] | [ ] | > \alpha | \ ] | ||||||||||
| 7 | hyperbolic cosine | [ \cosh(\alpha t) \cdot u(t) \ ] | [ ] | > \alpha | \ ] | ||||||||||
| 8 | Exponentially-decaying sine wave | [e^ \sin(\omega t) \cdot u(t) \ ] | [ ] | [ s > -\alpha \ ] | ||||||||||
| 9 | Exponentially-decaying cosine wave | [e^ \cos(\omega t) \cdot u(t) \ ] | [ ] | [ s > -\alpha \ ] | ||||||||||
| 10 | nth root | [ \sqrt[n] \cdot u(t) ] | [ s^ \cdot \Gamma\left(1+\frac\right)] | [ s > 0 \, ] | ||||||||||
| 11 | natural logarithm | [ \ln \left ( \right ) \cdot u(t) ] | [ - \ [ 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\right)^}}] | [ s > 0 \, ] [ (n > -1) \, ] | ||||||||||
| 13 | Modified Bessel function of the first kind, of order n | [I_n(\omega t) \cdot u(t)] | [ \frac\right)^}} ] | > \omega | \, ] | ||||||||||
| 14 | Bessel function of the second kind, of order 0 | [ Y_0(\alpha t) \cdot u(t)] | ||||||||||||
| 15 | Modified Bessel function of the second kind, of order 0 | [ K_0(\alpha t) \cdot u(t)] | ||||||||||||
| 16 | Error function | [ \mathrm(t) \cdot u(t) ] | [ \operatorname \left(s/2\right) \over s}] | [ s > 0 \, ] | ||||||||||
Explanatory notes:
s-Domain equivalent circuits and impedancesThe 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. However, s-Domain impedances are valid for many more inputs than 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 theoremsThe 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.
Example #1: Solving a differential equation
We can use the Laplace transform to solve this equation. Rearranging the equation to one side, we have
Example #2: Deriving the complex impedance for a capacitor
Taking the Laplace transform of this equation, we obtain
Example #3: Finding the transfer function from the impulse response
Suppose that we want to find the transfer function of the system. We begin by noting that
The transfer function is simply the Laplace transform of the impulse response:
Example #4: Method of partial fraction expansionConsider a linear time-invariant system with transfer function
The impulse response is simply the inverse Laplace transform of this transfer function:
To evaluate this inverse transform, we begin by expanding H(s) using the method of partial fraction expansion:
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:
Example #5: Mixing sines, cosines, and exponentials
Starting with the Laplace transform,
Example #6: Phase delay
Starting with the Laplace transform, [X(s) = \frac] we find the inverse by first by rearranging terms in the fraction: [X(s) = \frac + \frac]
[x(t) = (\sin \phi) \mathcal^\left\ \right\} + (\cos \phi) \mathcal^\left\ \right\}]
To simplify this answer, we must recall the trigonometric identity that [a \sin \omega t + b \cos \omega t = \sqrt \cdot \sin \left(\omega t + \arctan (b/a) \right)] and apply it to our value for x(t): [x(t) = \sqrt \cdot \sin \left( \omega t + \arctan \left(\frac \right) \right)]
We can apply similar logic to find that [\mathcal^ \left\ \right\} = \cos]. References
See also
External links
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