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词条 Laplace transform
释义

  1. History

  2. Formal definition

      Bilateral Laplace transform    Inverse Laplace transform    Probability theory  

  3. Region of convergence

  4. Properties and theorems

      Relation to power series    Relation to moments    Proof of the Laplace transform of a function's derivative    Evaluating integrals over the positive real axis    Relationship to other transforms    Laplace–Stieltjes transform    Fourier transform    Mellin transform    Z-transform    Borel transform    Fundamental relationships  

  5. Table of selected Laplace transforms

  6. s-domain equivalent circuits and impedances

  7. Examples and applications

      Evaluating improper integrals    Nuclear physics    Complex impedance of a capacitor    Partial fraction expansion    Phase delay    {{Anchor|Inferring spatial structure from spectrum}}Determining structure of astronomical object from spectrum    Statistical mechanics  

  8. See also

  9. Notes

  10. References

      Modern    Historical  

  11. Further reading

  12. External links

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In mathematics, the Laplace transform is an integral transform named after its inventor Pierre-Simon Laplace ({{IPAc-en|l|ə|ˈ|p|l|ɑ:|s}}). It takes a function of a real variable {{math|t}} (often time) to a function of a complex variable {{mvar|s}} (complex frequency).

The Laplace transform is similar to the Fourier transform. While the Fourier transform of a function is a complex function of a real variable (frequency), the Laplace transform of a function is a complex function of a complex variable. Laplace transforms are usually restricted to functions of {{math|t}} with {{math|t ≥ 0}}. A consequence of this restriction is that the Laplace transform of a function is a holomorphic function of the variable {{math|s}}. Unlike the Fourier transform, the Laplace transform of a distribution is generally a well-behaved function. Techniques of complex variables can also be used to directly study Laplace transforms. As a holomorphic function, the Laplace transform has a power series representation. This power series expresses a function as a linear superposition of moments of the function. This perspective has applications in probability theory.

The Laplace transform is invertible on a large class of functions. The inverse Laplace transform takes a function of a complex variable s (often frequency) and yields a function of a real variable t (often 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.[1] So, for example, Laplace transformation from the time domain to the frequency domain transforms differential equations into algebraic equations and convolution into multiplication. It has many applications in the sciences and technology.

History

The Laplace transform is named after mathematician and astronomer Pierre-Simon Laplace, who used a similar transform in his work on probability theory.[2] Laplace's use of generating functions was similar to what is now known as the z-transform and he gave little attention to the continuous variable case which was discussed by Abel.[3] The theory was further developed in the 19th and early 20th centuries by Lerch,[4] Heaviside,[5] and Bromwich.[6] The current widespread use of the transform (mainly in engineering) came about during and soon after World War II[7] replacing the earlier Heaviside operational calculus. The advantages of the Laplace transform had been emphasized by Doetsch[8] to whom the name Laplace Transform is apparently due.

The early history of methods having some similarity to Laplace transform is as follows. From 1744, Leonhard Euler investigated integrals of the form

as solutions of differential equations but did not pursue the matter very far.[9]

Joseph Louis Lagrange was an admirer of Euler and, in his work on integrating probability density functions, investigated expressions of the form

which some modern historians have interpreted within modern Laplace transform theory.[10][11]{{Clarify|date=May 2010}}

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.[12] However, in 1785, Laplace took the critical step forward when, rather than just looking 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

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.[13]

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 because those solutions were periodic. In 1809, Laplace applied his transform to find solutions that diffused indefinitely in space.[14]

Formal definition

The Laplace transform of a function {{math|f(t)}}, defined for all real numbers {{math|t ≥ 0}}, is the function {{math|F(s)}}, which is a unilateral transform defined by

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where s is a complex number frequency parameter

, with real numbers {{math|σ}} and {{math|ω}}.

An alternate notation for the Laplace transform is instead of {{math|F}}.

The meaning of the integral depends on types of functions of interest. A necessary condition for existence of the integral is that {{math|f}} must be locally integrable on {{closed-open|0, ∞}}. For locally integrable functions that decay at infinity or are of exponential type, the integral can be understood to be a (proper) Lebesgue integral. However, for many applications it is necessary to regard it as a conditionally convergent improper integral at {{math|∞}}. Still more generally, the integral can be understood in a weak sense, and this is dealt with below.

One can define the Laplace transform of a finite Borel measure {{math|μ}} by the Lebesgue integral[15]

An important special case is where {{math|μ}} is a probability measure, for example, the Dirac delta function. In operational calculus, the Laplace transform of a measure is often treated as though the measure came from a probability density function {{math|f}}. In that case, to avoid potential confusion, one often writes

where the lower limit of {{math|0}} is shorthand notation for

This limit emphasizes that any point mass located at {{math|0}} is entirely captured by the Laplace transform. Although with the Lebesgue integral, it is not necessary to take such a limit, it does appear more naturally in connection with the Laplace–Stieltjes transform.

Bilateral Laplace transform

{{Main article|Two-sided 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:

{{math|F(s)}}, which is a unilateral transform defined by{{Equation box 1
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An alternate notation for the bilateral Laplace transform is instead of .

Inverse Laplace transform

{{Main article|Inverse Laplace transform}}

Two integrable functions have the same Laplace transform only if they differ on a set of Lebesgue measure zero. This means that, on the range of the transform, there is an inverse transform. In fact, besides integrable functions, the Laplace transform is a one-to-one mapping from one function space into another in many other function spaces as well, although there is usually no easy characterization of the range. Typical function spaces in which this is true include the spaces of bounded continuous functions, the space {{math|L(0, ∞)}}, or more generally tempered distributions on {{open-open|0, ∞}}. The Laplace transform is also defined and injective for suitable spaces of tempered distributions.

In these cases, the image of the Laplace transform lives in a space of analytic functions in the region of convergence. 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):

The bilateral Laplace transform is defined as follows:

{{math|F(s)}}, which is a unilateral transform defined by{{Equation box 1
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where {{math|γ}} is a real number so that the contour path of integration is in the region of convergence of {{math|F(s)}}. An alternative formula for the inverse Laplace transform is given by Post's inversion formula. The limit here is interpreted in the weak-* topology.

In practice, it is typically more convenient to decompose a Laplace transform into known transforms of functions obtained from a table, and construct the inverse by inspection.

Probability theory

In pure and applied probability, the Laplace transform is defined as an expected value. If {{math|X}} is a random variable with probability density function {{math|f}}, then the Laplace transform of {{math|f}} is given by the expectation

By convention, this is referred to as the Laplace transform of the random variable {{math|X}} itself. Replacing {{math|s}} by {{math|−t}} gives the moment generating function of {{math|X}}. The Laplace transform has applications throughout probability theory, including first passage times of stochastic processes such as Markov chains, and renewal theory.

Of particular use is the ability to recover the cumulative distribution function of a continuous random variable {{math|X}} by means of the Laplace transform as follows[16]

Region of convergence

If {{math|f}} is a locally integrable function (or more generally a Borel measure locally of bounded variation), then the Laplace transform {{math|F(s)}} of {{math|f}} converges provided that the limit

exists.

The Laplace transform converges absolutely if the integral

exists (as a proper Lebesgue integral). The Laplace transform is usually understood as conditionally convergent, meaning that it converges in the former instead of the latter sense.

The set of values for which {{math|F(s)}} converges absolutely is either of the form {{math|Re(s) > a}} or else {{math|Re(s) ≥ a}}, where {{math|a}} is an extended real constant, {{math|−∞ ≤ a ≤ ∞}}. (This follows from the dominated convergence theorem.) The constant {{math|a}} is known as the abscissa of absolute convergence, and depends on the growth behavior of {{math|f(t)}}.[17] Analogously, the two-sided transform converges absolutely in a strip of the form {{math|a < Re(s) < b}}, and possibly including the lines {{math|1=Re(s) = a}} or {{math|1=Re(s) = b}}.[18] The subset of values of {{math|s}} for which the Laplace transform converges absolutely is called the region of absolute convergence or the domain of absolute convergence. In the two-sided case, it is sometimes called the strip of absolute convergence. The Laplace transform is analytic in the region of absolute convergence: this is a consequence of Fubini's theorem and Morera's theorem.

Similarly, the set of values for which {{math|F(s)}} converges (conditionally or absolutely) is known as the region of conditional convergence, or simply the region of convergence (ROC). If the Laplace transform converges (conditionally) at {{math|1=s = s0}}, then it automatically converges for all {{math|s}} with {{math|Re(s) > Re(s0)}}. Therefore, the region of convergence is a half-plane of the form {{math|Re(s) > a}}, possibly including some points of the boundary line {{math|1=Re(s) = a}}.

In the region of convergence {{math|Re(s) > Re(s0)}}, the Laplace transform of {{math|f}} can be expressed by integrating by parts as the integral

That is, in the region of convergence {{math|F(s)}} can effectively be expressed as the absolutely convergent Laplace transform of some other function. In particular, it is analytic.

There are several Paley–Wiener theorems concerning the relationship between the decay properties of {{math|f}} and the properties of the Laplace transform within the region of convergence.

In engineering applications, a function corresponding to a linear time-invariant (LTI) system is stable if every bounded input produces a bounded output. This is equivalent to the absolute convergence of the Laplace transform of the impulse response function in the region {{math|Re(s) ≥ 0}}. As a result, LTI systems are stable provided the poles of the Laplace transform of the impulse response function have negative real part.

This ROC is used in knowing about the causality and stability of a system.

Properties and theorems

The Laplace transform has a number of properties that make it useful for analyzing linear dynamical systems. The most significant advantage is that differentiation and integration become multiplication and division, respectively, by {{math|s}} (similarly to logarithms changing multiplication of numbers to addition of their logarithms).

Because of this property, the Laplace variable {{math|s}} is also known as operator variable in the {{math|L}} domain: either derivative operator or (for {{math|s−1)}} integration operator. The transform turns integral equations and differential equations to polynomial equations, which are much easier to solve. Once solved, use of the inverse Laplace transform reverts to the original domain.

Given the functions {{math|f(t)}} and {{math|g(t)}}, and their respective Laplace transforms {{math|F(s)}} and {{math|G(s)}},

The following table is a list of properties of unilateral Laplace transform:[19]

 ! ! Time domain ! {{math|''s''}} domain ! Comment
Properties of the unilateral Laplace transform
Can be proved using basic rules of integration.
F′}} is the first derivative of {{math|F}} with respect to {{math|s}}.
n}}th derivative of {{math|F(s)}}.
f}} is assumed to be a differentiable function, and its derivative is assumed to be of exponential type. This can then be obtained by integration by parts
f}} is assumed twice differentiable and the second derivative to be of exponential type. Follows by applying the Differentiation property to {{math|f′(t)}}.
f}} is assumed to be {{math|n}}-times differentiable, with {{math|n}}th derivative of exponential type. Follows by mathematical induction.
This is deduced using the nature of frequency differentiation and conditional convergence.
u(t)}} is the Heaviside step function and {{math|(u ∗ f)(t)}} is the convolution of {{math|u(t)}} and {{math|f(t)}}.
u(t)}} is the Heaviside step function
1=Re(σ) = c}} that lies entirely within the region of convergence of {{math|F}}.[20]
f(t)}} is a periodic function of period {{math|T}} so that {{math|1=f(t) = f(t + T)}}, for all {{math|t ≥ 0}}. This is the result of the time shifting property and the geometric series.
  • Initial value theorem:

  • Final value theorem:

, if all poles of sF(s) are in the left half-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 {{math|F(s)}} has a pole in the right-hand plane or poles on the imaginary axis (e.g., if or ), the behaviour of this formula is undefined.

Relation to power series

The Laplace transform can be viewed as a continuous analogue of a power series. If {{math|a(n)}} is a discrete function of a positive integer {{math|n}}, then the power series associated to {{math|a(n)}} is the series

where {{math|x}} is a real variable (see Z transform). Replacing summation over {{math|n}} with integration over {{math|t}}, a continuous version of the power series becomes

where the discrete function {{math|a(n)}} is replaced by the continuous one {{math|f(t)}}.

Changing the base of the power from {{math|x}} to {{math|e}} gives

For this to converge for, say, all bounded functions {{math|f}}, it is necessary to require that {{math|ln x < 0}}. Making the substitution {{math|1=−s = ln x}} gives just the Laplace transform:

In other words, the Laplace transform is a continuous analog of a power series in which the discrete parameter {{math|n}} is replaced by the continuous parameter {{math|t}}, and {{math|x}} is replaced by {{math|es}}.

Relation to moments

{{main article|Moment generating function}}

The quantities

are the moments of the function {{math|f}}. If the first {{math|n}} moments of {{math|f}} converge absolutely, then by repeated differentiation under the integral,

This is of special significance in probability theory, where the moments of a random variable {{math|X}} are given by the expectation values . Then, the relation holds

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:

yielding

and in the bilateral case,

The general result

where denotes the {{math|n}}th derivative of {{math|f}}, can then be established with an inductive argument.

Evaluating integrals over the positive real axis

A useful property of the Laplace transform is the following:

under suitable assumptions on the behaviour of in a right neighbourhood of and on the decay rate of in a left neighbourhood of . The above formula is a variation of integration by parts, with the operators

and being replaced by and . Let us prove the equivalent formulation:

By plugging in the left-hand side turns into:

but assuming Fubini's theorem holds, by reversing the order of integration we get the wanted right-hand side.

Relationship to other transforms

Laplace–Stieltjes transform

The (unilateral) Laplace–Stieltjes transform of a function {{math|g : RR}} is defined by the Lebesgue–Stieltjes integral

The function {{math|g}} is assumed to be of bounded variation. If {{math|g}} is the antiderivative of {{math|f}}:

then the Laplace–Stieltjes transform of {{math|g}} and the Laplace transform of {{math|f}} coincide. In general, the Laplace–Stieltjes transform is the Laplace transform of the Stieltjes measure associated to {{math|g}}. So in practice, the only distinction between the two transforms is that the Laplace transform is thought of as operating on the density function of the measure, whereas the Laplace–Stieltjes transform is thought of as operating on its cumulative distribution function.[21]

Fourier transform

The continuous Fourier transform is equivalent to evaluating the bilateral Laplace transform with imaginary argument {{math|1=s = }} or {{math|1=s = 2πfi}}[22] when the condition explained below is fulfilled,

This definition of the Fourier transform requires a prefactor of 1/2 {{math|π}} on the reverse Fourier transform. This relationship between the Laplace and Fourier transforms is often used to determine the frequency spectrum of a signal or dynamical system.

The above relation is valid as stated if and only if the region of convergence (ROC) of {{math|F(s)}} contains the imaginary axis, {{math|1=σ = 0}}.

For example, the function {{math|1=f(t) = cos(ω0t)}} has a Laplace transform {{math|1=F(s) = s/(s2 + ω02)}} whose ROC is {{math|Re(s) > 0}}. As {{math|1=s = }} is a pole of {{math|F(s)}}, substituting {{math|1=s = }} in {{math|F(s)}} does not yield the Fourier transform of {{math|f(t)u(t)}}, which is proportional to the Dirac delta-function {{math|δ(ωω0)}}.

However, a relation of the form

holds under much weaker conditions. For instance, this holds for the above example provided that the limit is understood as a weak limit of measures (see vague topology). General conditions relating the limit of the Laplace transform of a function on the boundary to the Fourier transform take the form of Paley–Wiener theorems.

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

we set {{math|1=θ = et}} we get a two-sided Laplace transform.

Z-transform

The unilateral or one-sided Z-transform is simply the Laplace transform of an ideally sampled signal with the substitution of

where {{math|1=T = 1/fs}} is the sampling period (in units of time e.g., seconds) and {{math|fs}} is the sampling rate (in samples per second or hertz).

Let

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

be the sampled representation of the continuous-time {{math|x(t)}}

The Laplace transform of the sampled signal {{math|xq(t)}} is

This is the precise definition of the unilateral Z-transform of the discrete function {{math|x[n]}}

with the substitution of {{math|z → esT}}.

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

The similarity between the {{math|Z}} and Laplace transforms is expanded upon in the theory of time scale calculus.

Borel transform

The integral form of the Borel transform

is a special case of the Laplace transform for {{math|f}} an entire function of exponential type, meaning that

for some constants {{math|A}} and {{math|B}}. The generalized Borel transform allows a different weighting function to be used, rather than the exponential function, to transform functions not of exponential type. Nachbin's theorem gives necessary and sufficient conditions for the Borel transform to be well defined.

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

{{main article|List of Laplace transforms}}

The following table provides Laplace transforms for many common functions of a single variable.[23][24] 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.

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

Using this linearity, and various trigonometric, hyperbolic, and complex number (etc.) properties and/or identities, some Laplace transforms can be obtained from others more quickly than by using the definition directly.

The unilateral Laplace transform takes as input a function whose time domain is the non-negative reals, which is why all of the time domain functions in the table below are multiples of the Heaviside step function, {{math|u(t)}}.

The entries of the table that involve a time delay {{math|τ}} are required to be causal (meaning that {{math|τ > 0}}). A causal system is a system where the impulse response {{math|h(t)}} is zero for all time {{mvar|t}} prior to {{math|1=t = 0}}. In general, the region of convergence for causal systems is not the same as that of anticausal systems.

Function Time domain
s-domain
Region of convergence Reference
unit impulseall {{math|s}}inspection
delayed impulsetime shift of
unit impulse
unit step{{math|Re(s) > 0}}integrate unit impulse
delayed unit step{{math|Re(s) > 0}}time shift of
unit step
ramp{{math|Re(s) > 0}}integrate unit
impulse twice
n}}th power
(for integer {{math|n}})
{{math|Re(s) > 0}}
({{math|n > −1}})
Integrate unit
step {{math|n}} times
q}}th power
(for complex {{math|q}})
{{math|Re(s) > 0}}
{{math|Re(q) > −1}}
[25][26]
n}}th root{{math|Re(s) > 0}}Set {{math|1=q = 1/n}} above.
n}}th power with frequency shift{{math|Re(s) > −α}}Integrate unit step,
apply frequency shift
n}}th power
with frequency shift
{{math|Re(s) > −α}}Integrate unit step,
apply frequency shift,
apply time shift
exponential decay{{math|Re(s) > −α}}Frequency shift of
unit step
two-sided exponential decay
(only for bilateral transform)
{{math|−α < Re(s) < α}}Frequency shift of
unit step
exponential approach{{math|Re(s) > 0}}Unit step minus
exponential decay
sine{{math|Re(s) > 0}}{{Harvnb|Bracewell|1978|p=227}}
cosine{{math|Re(s) > 0}}{{Harvnb|Bracewell|1978|p=227}}
hyperbolic sine{{math|Re(s) > {{abs|α}}}}{{Harvnb|Williams|1973|p=88}}
hyperbolic cosine{{math|Re(s) > {{abs|α}}}}{{Harvnb|Williams|1973|p=88}}
exponentially decaying
sine wave
{{math|Re(s) > −α}}{{Harvnb|Bracewell|1978|p=227}}
exponentially decaying
cosine wave
{{math|Re(s) > −α}}{{Harvnb|Bracewell|1978|p=227}}
natural logarithm{{math|Re(s) > 0}}{{Harvnb|Williams|1973|p=88}}
Bessel function
of the first kind,
of order n
{{math|Re(s) > 0}}
({{math|n > −1}})
{{Harvnb|Williams|1973|p=89}}
Error function{{math|Re(s) > 0}}{{Harvnb|Williams|1973|p=89}}
Explanatory notes:{{col-begin}}{{col-break}}
  • {{math|u(t)}} represents the Heaviside step function.
  • {{math|δ}} represents the Dirac delta function.
  • {{math|Γ(z)}} represents the Gamma function.
  • {{math|γ}} is the Euler–Mascheroni constant.
{{col-break}}
  • {{math|t}}, a real number, typically represents time,
    although it can represent any independent dimension.
  • {{math|s}} is the complex frequency domain parameter, and {{math|Re(s)}} is its real part.
  • {{math|α, β, τ, and ω}} are real numbers.
  • {{math|n}} is an integer.
{{col-end}}

s-domain equivalent circuits and impedances

The Laplace transform is often used in circuit analysis, and simple conversions to the {{math|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 {{math|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 {{math|s}}-domain account for that.

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

Examples and applications

The Laplace transform is used frequently in engineering and physics; the output of a linear time-invariant 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 mechanical engineering and electrical engineering. The Laplace transform reduces a linear differential equation to an algebraic equation, which can then be solved by the formal rules of algebra. The original differential equation can then be solved by applying the inverse Laplace transform. The English electrical engineer Oliver Heaviside first proposed a similar scheme, although without using the Laplace transform; and the resulting operational calculus is credited as the Heaviside calculus.

Evaluating improper integrals

Let , then (see the table above)

or

Letting {{math|s → 0}}, gives one the identity

provided that the interchange of limits can be justified. Even when the interchange cannot be justified the calculation can be suggestive. For example, proceeding formally one has

The validity of this identity can be proved by other means. It is an example of a Frullani integral.

Another example is Dirichlet integral.

Nuclear physics

In nuclear physics, the following fundamental relationship governs radioactive decay: the number of radioactive atoms {{math|N}} in a sample of a radioactive isotope decays at a rate proportional to {{math|N}}. This leads to the first order linear differential equation

where {{math|λ}} is the decay constant. The Laplace transform can be used to solve this equation.

Rearranging the equation to one side, we have

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

where

and

Solving, we find

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

which is indeed the correct form for radioactive decay.

Complex impedance of a capacitor

In the theory of electrical circuits, the current flow in a capacitor is proportional to the capacitance and rate of change in the electrical potential (in SI units). Symbolically, this is expressed by the differential equation

where {{math|C}} is the capacitance (in farads) of the capacitor, {{math|1=i = i(t)}} is the electric current (in amperes) through the capacitor as a function of time, and {{math|1=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

where

and

Solving for {{math|V(s)}} we have

The definition of the complex impedance {{math|Z}} (in ohms) is the ratio of the complex voltage {{math|V}} divided by the complex current {{math|I}} while holding the initial state {{math|V0}} at zero:

Using this definition and the previous equation, we find:

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

In addition, the Laplace transform has large applications in control theory.

Partial fraction expansion

Consider 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 {{math|H(s)}} using the method of partial fraction expansion,

The unknown constants {{math|P}} and {{math|R}} are the residues located at the corresponding poles of the transfer function. Each residue represents the relative contribution of that singularity to the transfer function's overall shape.

By the residue theorem, the inverse Laplace transform depends only upon the poles and their residues. To find the residue {{math|P}}, we multiply both sides of the equation by {{math|s + α}} to get

Then by letting {{math|1=s = −α}}, the contribution from {{math|R}} vanishes and all that is left is

Similarly, the residue {{math|R}} is given by

Note that

and so the substitution of {{math|R}} and {{math|P}} into the expanded expression for {{math|H(s)}} gives

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 {{math|H(s)}} to obtain

which is the impulse response of the system.

Convolution

The same result can be achieved using the convolution property as if the system is a series of filters with transfer functions of {{math|1/(s + a)}} and {{math|1/(s + b)}}. That is, the inverse of

is

Phase delay

Time function Laplace transform

Starting with the Laplace transform,

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

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

This is just the sine of the sum of the arguments, yielding:

We can apply similar logic to find that

{{Anchor|Inferring spatial structure from spectrum}}Determining structure of astronomical object from spectrum

The wide and general applicability of the Laplace transform and its inverse is illustrated by an application in astronomy which provides some information on the spatial distribution of matter of an astronomical source of radio-frequency thermal radiation too distant to resolve as more than a point, given its flux density spectrum, rather than relating the time domain with the spectrum (frequency domain).

Assuming certain properties of the object, e.g. spherical shape and constant temperature, calculations based on carrying out an inverse Laplace transformation on the spectrum of the object can produce the only possible model of the distribution of matter in it (density as a function of distance from the center) consistent with the spectrum.[27] When independent information on the structure of an object is available, the inverse Laplace transform method has been found to be in good agreement.

Statistical mechanics

In statistical mechanics, the Laplace transform of the density of states defines the partition function.[28] That is, the partition function is given by

and the inverse is given by

See also

{{div col}}
  • Analog signal processing
  • Bernstein's theorem on monotone functions
  • Continuous-repayment mortgage
  • Fourier transform
  • Hamburger moment problem
  • Hardy–Littlewood tauberian theorem
  • Laplace–Carson transform
  • Moment-generating function
  • Pierre-Simon Laplace
  • Post's inversion formula
  • Signal-flow graph
  • Symbolic integration
  • Transfer function
  • Z-transform (discrete equivalent of the Laplace transform)
{{div col end}}

Notes

1. ^{{harvnb|Korn|Korn|1967|loc=§8.1}}
2. ^{{citation |url=https://archive.org/details/thorieanalytiqu01laplgoog |title=Théorie analytique des Probabilités |location=Paris |date=1814 |edition=2nd |at=chap.I sect.2-20 |chapter=Des Fonctions génératrices |trans-title=Analytical Probability Theory |trans-chapter=On generating functions |language=fr}}
3. ^{{citation |first=N. H. |last=Abel |chapter=Sur les fonctions génératrices et leurs déterminantes |date=1820 |title=Œuvres Complètes |language=fr |publication-date=1839 |volume=II |pages=77–88}} [https://books.google.com/books?id=6FtDAQAAMAAJ&pg=RA2-PA67&lpg=RA2-PA67 1881 edition]
4. ^{{citation |first=M. |last=Lerch |author-link=Mathias Lerch |title=Sur un point de la théorie des fonctions génératrices d'Abel |journal=Acta Math. |volume=27 |date=1903 |pages=339–351 |url=https://projecteuclid.org/euclid.acta/1485882168 |doi=10.1007/BF02421315 |trans-title=Proof of the inversion formula |language=fr}}
5. ^{{citation |first=O. |last=Heaviside |author-link=Oliver Heaviside |chapter=The solution of definite integrals by differential transformation |title=Electromagnetic Theory |location=London |at=section 526 |volume=III |chapter-url=https://books.google.com/books?id=y9auR0L6ZRcC&pg=PA234&lpg=PA234|isbn=9781605206189 |date=January 2008 }}
6. ^{{citation |first=T. J. |last=Bromwich |author-link=Thomas John I'Anson Bromwich |title=Normal coordinates in dynamical systems |journal=Proc. London Math. Soc. |volume=15 |pages=401–448 |date=1916 |doi=10.1112/plms/s2-15.1.401}}
7. ^An influential book was: {{citation |first=M. F. |last=Gardner |first2=J. L. |last2=Barnes |title=Transients in Linear Systems studied by the Laplace Transform |date=1942 |location=New York |publisher=Wiley}}
8. ^{{citation |first=G. |last=Doetsch |title=Theorie und Anwendung der Laplacesche Transformation |location=Berlin |date=1937 |publisher=Springer |language=de |trans-title=Theory and Application of the Laplace Transform}} translation 1943
9. ^{{harvnb|Euler|1744}}, {{harvnb|Euler|1753}}, {{harvnb|Euler|1769}}
10. ^{{harvnb|Lagrange|1773}}
11. ^{{harvnb|Grattan-Guinness| 1997|p=260}}
12. ^{{harvnb|Grattan-Guinness|1997|p=261}}
13. ^{{harvnb|Grattan-Guinness|1997|pp=261–262}}
14. ^{{harvnb|Grattan-Guinness|1997|pp=262–266}}
15. ^{{harvnb|Feller|1971|loc=§XIII.1}}
16. ^The cumulative distribution function is the integral of the probability density function.
17. ^{{harvnb|Widder|1941|loc=Chapter II, §1}}
18. ^{{harvnb|Widder|1941|loc=Chapter VI, §2}}
19. ^{{harvnb|Korn|Korn|1967|pp=226–227}}
20. ^{{harvnb|Bracewell|2000|loc=Table 14.1, p. 385}}
21. ^{{harvnb|Feller|1971|p=432}}
22. ^{{harvnb|Takacs|1953|p=93}}
23. ^{{Citation |edition=3rd |page=455 |first1=K. F. |last1=Riley |first2=M. P. |last2=Hobson |first3=S. J. |last3=Bence |title=Mathematical methods for physics and engineering |publisher=Cambridge University Press |year=2010 |isbn=978-0-521-86153-3}}
24. ^{{Citation |first1=J. J. |last1=Distefano |first2=A. R. |last2=Stubberud |first3=I. J. |last3=Williams |page=78 |title=Feedback systems and control |edition=2nd |publisher=McGraw-Hill |series=Schaum's outlines |year=1995 |isbn=978-0-07-017052-0}}
25. ^{{citation |title=Mathematical Handbook of Formulas and Tables |edition=3rd |first1=S. |last1=Lipschutz |first2=M. R. |last2=Spiegel |first3=J. |last3=Liu |series=Schaum's Outline Series |publisher=McGraw-Hill |page=183 |year=2009 |isbn=978-0-07-154855-7}} – provides the case for real {{math|q}}.
26. ^http://mathworld.wolfram.com/LaplaceTransform.html – Wolfram Mathword provides case for complex {{math|q}}
27. ^{{citation |first1=M. |last1=Salem |first2=M. J. |last2=Seaton |year=1974 |url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974MNRAS.167..493S&link_type=ARTICLE&db_key=AST&high= |title=I. Continuum spectra and brightness contours |journal=Monthly Notices of the Royal Astronomical Society |volume=167 |issue=3 |pages=493–510 |doi=10.1093/mnras/167.3.493 |bibcode=1974MNRAS.167..493S}}, and
{{citation |first1=M. |last1=Salem |year=1974 |url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974MNRAS.167..511S&link_type=ARTICLE&db_key=AST&high= |title=II. Three-dimensional models |journal=Monthly Notices of the Royal Astronomical Society |volume=167 |issue=3 |pages=511–516 |doi=10.1093/mnras/167.3.511 |bibcode=1974MNRAS.167..511S}}
28. ^{{cite book|author1=RK Pathria|author2=Paul Beal|title=Statistical mechanics|edition=2nd|publisher=Butterworth-Heinemann|year=1996|page=56}}

References

Modern

  • {{Citation |last=Bracewell |first=Ronald N. |title=The Fourier Transform and its Applications |edition=2nd |year=1978 |publisher=McGraw-Hill Kogakusha |isbn=978-0-07-007013-4 }}
  • {{citation|first=R. N.|last=Bracewell|title=The Fourier Transform and Its Applications|edition=3rd|location=Boston|publisher=McGraw-Hill|year=2000|isbn=978-0-07-116043-8}}
  • {{Citation | last1=Feller | first1=William | author1-link=William Feller | title=An introduction to probability theory and its applications. Vol. II. | publisher=John Wiley & Sons | location=New York | series=Second edition | mr=0270403 | year=1971}}
  • {{citation |first1=G. A. |last1=Korn |first2=T. M. |last2=Korn |title=Mathematical Handbook for Scientists and Engineers |publisher=McGraw-Hill Companies |edition=2nd |year=1967 |isbn=978-0-07-035370-1 }}
  • {{Citation | last1=Widder | first1=David Vernon | title=The Laplace Transform | publisher=Princeton University Press | series=Princeton Mathematical Series, v. 6 | mr=0005923 | year=1941}}
  • {{Citation | last=Williams |first=J. |title=Laplace Transforms |series=Problem Solvers |volume= |publisher=George Allen & Unwin |year=1973 |isbn= 978-0-04-512021-5 }}
  • {{Citation | last=Takacs | first= J.|title=Fourier amplitudok meghatarozasa operatorszamitassal | year=1953 | journal=Magyar Hiradastechnika | volume=IV | issue=7–8|pages=93–96 |language=Hungarian }}

Historical

  • {{citation |last=Euler |first=L. |authorlink=Leonhard Euler |year=1744 |title=De constructione aequationum |trans-title=The Construction of Equations |language=la |journal=Opera Omnia |series=1st series |volume=22 |pages=150–161}}
  • {{citation |last=Euler |first=L. |authorlink=Leonhard Euler |year=1753 |title=Methodus aequationes differentiales |trans-title=A Method for Solving Differential Equations |language=la |journal=Opera Omnia |series=1st series |volume=22 |pages=181–213}}
  • {{citation |last=Euler |first=L. |authorlink=Leonhard Euler |origyear=1769 |title=Institutiones calculi integralis, Volume 2 |trans-title=Institutions of Integral Calculus |language=la |journal=Opera Omnia |series=1st series |volume=12 |year=1992 |location=Basel |publisher=Birkhäuser |isbn=978-3764314743 }}, Chapters 3–5
  • {{citation |last=Euler |first=Leonhard |authorlink=Leonhard Euler |year=1769 |title=Institutiones calculi integralis |trans-title=Institutions of Integral Calculus |language=la |volume=II |at=ch. 3–5, pp. 57–153 |location=Paris |publisher=Petropoli |url=https://books.google.com/books?id=BFqWNwpfqo8C }}
  • {{citation|last=Grattan-Guinness|first=I|authorlink=Ivor Grattan-Guinness|year=1997|contribution=Laplace's integral solutions to partial differential equations|editor=Gillispie, C. C.|title=Pierre Simon Laplace 1749–1827: A Life in Exact Science|location=Princeton|publisher=Princeton University Press|isbn=978-0-691-01185-1}}
  • {{citation|last=Lagrange|first=J. L.|authorlink=Joseph Louis Lagrange|year=1773|title=Mémoire sur l'utilité de la méthode|series=Œuvres de Lagrange|volume=2|pages=171–234}}

Further reading

  • {{citation|first1=Wolfgang|last1=Arendt|first2=Charles J.K.|last2=Batty|first3=Matthias|last3=Hieber|first4=Frank|last4=Neubrander|title=Vector-Valued Laplace Transforms and Cauchy Problems|publisher=Birkhäuser Basel|year=2002|isbn=978-3-7643-6549-3 |ref=none}}.
  • {{citation|last=Davies|first=Brian|title=Integral transforms and their applications|edition=Third|publisher=Springer|location=New York|year=2002|isbn= 978-0-387-95314-4 |ref=none}}
  • {{citation | last=Deakin|first= M. A. B. | year=1981 | title=The development of the Laplace transform | journal=Archive for History of Exact Sciences | volume=25 | pages=343–390 | doi=10.1007/BF01395660 | issue=4 |ref=none}}
  • {{citation | last=Deakin|first= M. A. B. | year=1982 | title=The development of the Laplace transform | journal=Archive for History of Exact Sciences | volume=26 | pages=351–381 | doi=10.1007/BF00418754 | issue=4 |ref=none}}
  • {{citation |last=Doetsch |first=Gustav |authorlink=Gustav Doetsch |date=1974 |title=Introduction to the Theory and Application of the Laplace Transformation |publisher=Springer |isbn=978-0-387-06407-9 |ref=none}}
  • Mathews, Jon; Walker, Robert L. (1970), Mathematical methods of physics (2nd ed.), New York: W. A. Benjamin, {{isbn|0-8053-7002-1}}
  • {{citation|first1=A. D.|last1=Polyanin|first2=A. V.|last2=Manzhirov|title=Handbook of Integral Equations|publisher=CRC Press|location=Boca Raton|year=1998|isbn=978-0-8493-2876-3 |ref=none}}
  • {{Citation | last1=Schwartz | first1=Laurent | author-link=Laurent Schwartz | title=Transformation de Laplace des distributions | mr=0052555 | year=1952 | journal=Comm. Sém. Math. Univ. Lund [Medd. Lunds Univ. Mat. Sem.] | volume=1952 | pages=196–206 |language=French |ref=none}}
  • {{Citation |last=Schwartz |first=Laurent |author-link=Laurent Schwartz |year=2008 |origyear=1966 |title=Mathematics for the Physical Sciences |publisher=Dover Publications |location=New York |series=Dover Books on Mathematics |pages=215–241 |isbn=978-0-486-46662-0 |url={{Google books|-_AuDQAAQBAJ|Mathematics for the Physical Sciences|page=215|plainurl=yes}} |ref=none}} - See Chapter VI. The Laplace transform.
  • {{citation|first=William McC.|last=Siebert|title=Circuits, Signals, and Systems|publisher=MIT Press|location=Cambridge, Massachusetts|year=1986|isbn=978-0-262-19229-3 |ref=none}}
  • {{Citation | last1=Widder | first1=David Vernon | title=What is the Laplace transform? | mr=0013447 | year=1945 | journal=The American Mathematical Monthly | issn=0002-9890 |volume=52 |issue=8 | pages=419–425 | doi=10.2307/2305640 | jstor=2305640 |ref=none}}

External links

{{wikiquote}}{{commons category|Laplace transformation}}
  • {{springer|title=Laplace transform|id=p/l057540}}
  • Online Computation of the transform or inverse transform, wims.unice.fr
  • Tables of Integral Transforms at EqWorld: The World of Mathematical Equations.
  • {{MathWorld|title=Laplace Transform|urlname=LaplaceTransform}}
  • Good explanations of the initial and final value theorems
  • Laplace Transforms at MathPages
  • Computational Knowledge Engine allows to easily calculate Laplace Transforms and its inverse Transform.
  • Laplace Calculator to calculate Laplace Transforms online easily.
{{Authority control}}{{DEFAULTSORT:Laplace Transform}}

4 : Laplace transforms|Differential equations|Fourier analysis|Mathematical physics

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