An integral transform constructs a new function by integrating an input against a kernel:
The kernel specifies how each input location contributes to an output indexed by . Whenever the integrals exist, linearity gives . The function spaces, convergence conditions and normalization are part of the definition; a formal kernel alone need not define an invertible or even everywhere-defined linear operator.[ref]
The Laplace transform uses on nonnegative time. For it gives when . The Fourier transform decomposes a function into oscillatory frequencies, while the Mellin transform is adapted to changes of scale. A smoothing Gaussian kernel instead gives the Weierstrass transform.
The useful operation is often a change of representation: the Laplace transform of a derivative turns a constant-coefficient differential equation into an algebraic equation with initial data. The inverse step then requires a theorem, such as the Bromwich inversion formula, with its own regularity and convergence assumptions.
A family of integral transforms associated with a two-by-two real matrix of determinant one. For , one optical normalization has kernel proportional to . It includes free-space Fresnel diffraction, quadratic phase multiplication and the Fourier transform. The optical amplitude normalization in one transverse dimension is with a consistent phase branch.
The Weierstrass transform is Gaussian convolution, . It smooths appropriate functions and is the heat semigroup at unit time. The Brownian transition semigroup uses variance- Gaussian kernels and therefore supplies the scaled time family.
The spherical mean of a function on averages it over a sphere of radius about :
Here is surface measure on the unit sphere and is its total area. Using the unit sphere absorbs the physical surface-area factor into the change of variables. The expression requires an integrable restriction to that sphere; continuity near it is one sufficient condition.
For , expanding and using the zero average of gives . By contrast, the mean value property for harmonic functions gives when is harmonic on a neighborhood of the closed ball. Averaging over a boundary sphere and averaging over the whole ball are different operations, even though both have a mean-value property for harmonic functions.
In three dimensions let solve , where is supported in and . Write and . Outside , the weak solution is a harmonic function. The weak formulation against radial test functions gives for . The zero Sobolev trace gives ; integration proves the displayed formula, without assuming the source is a radial function.
Cauchy-Schwarz inequality on spheres gives . For fixed nonzero and fixed , this grows linearly in . Such solutions on expanding balls cannot remain bounded in the full norm after zero extension of H01.
The Radon transform integrates a function over affine hyperplanes:
The Radon transform records line integrals of a planar density. Apply the transverse Hilbert transform and a derivative to each projection, then average the filtered values over all lines through the reconstruction point. With , the filter has Fourier multiplier . The Fourier inversion theorem, or the jump of the complexified transport Cauchy kernel, proves the displayed formula. The factor is when directions are integrated over a half-circle. The growing Fourier multiplier explains amplification of measurement noise and the need for regularization of an inverse problem.
The integral of a source over a directed line, weighted by exponential absorption between each source point and a detector. For line coordinates and a detector at the negative end, it is . The integrating factor of a transport equation derives the weight. Reversing the detector direction changes the weight for spatially varying attenuation, so the two directed measurements need not coincide. Setting recovers the Radon transform.
For known attenuation and a scalar source in the plane, start with the directional transport equation . Introduce a complex spectral parameter and Wirtinger derivatives , :
At this is the original directional derivative . Away from the unit circle, its fundamental solution supplies analytic spectral families. Choosing with turns into , removing attenuation by an integrating factor.[ref]
The boundary values from inside and outside the unit circle have a jump determined by directed attenuated Radon transform data and transverse Hilbert transforms. A normalized Riemann-Hilbert problem reconstructs the spectral family. In the exterior normalization , substituting into the transformed equation gives . Thus the desired source is recovered from a spectral coefficient, rather than from a direct angular average.
This construction assumes sufficient regularity and decay, known attenuation and the required directed angular measurements. General angle-dependent sources have a different identifiable content; partial angular data require additional hypotheses. The projection formula for inverse attenuated Radon transform makes one full-data normalization explicit.
Let , , and be the directed attenuated Radon transform. With the signed Cauchy boundary operators, set . An integrating factor turns the attenuated equation into unattenuated directional transport; its spectral solution has jump on the unit circle. A normalized Cauchy integral formula and the coefficient at spectral infinity then prove the reconstruction formula. Known attenuation and full directed angular data determine the source; attenuation itself is not reconstructed by this pair.
For and , the operator has the displayed decaying fundamental solution. A rotated real-linear coordinate turns it into a multiple of a Wirtinger derivative, reducing the kernel identity to . The kernel is analytic in separately inside and outside the unit circle, is at zero and at infinity, and develops a jump at the real directional-transport limit.
The Mellin transform is an integral transform suited to changes of scale: replacing by multiplies its transform by for . For a locally integrable function , define
where the improper integral converges. The complex number uses the real natural logarithm because . Its absolute value is , so absolute convergence depends on the real part rather than the imaginary part . The Mellin fundamental strip records the open range of such real parts.[ref]
A familiar example is the exponential function :
This is exactly the Gamma integral. Near zero tends to one, so absolute convergence requires ; at infinity for every real , so there is no upper boundary. The Gamma function has a meromorphic continuation with simple poles at , but a finite continued value elsewhere in does not make the defining improper integral converge.[ref]
This is the Mellin transform of the function extended by zero beyond the unit interval. The change of variables identifies it with the unilateral Laplace transform of . The Bromwich inversion formula therefore gives for , with in the convergence half-plane and suitable inversion hypotheses. At a jump, symmetric inversion returns the mean of the two limiting values. In particular, for , the cutoff has transform when . Multiplication by shifts the support threshold in logarithmic coordinates, the Laplace transform time-shift rule expressed multiplicatively.
For real and , the displayed improper integral converges: its endpoint powers are near zero and near infinity. The change of variables gives
Here the beta function, the beta-gamma identity, and the Gamma reflection formula evaluate the integral. The same formula holds for complex in the Mellin fundamental strip , by absolute convergence and analytic continuation within the strip. For integer , a sector contour of angle gives a direct residue theorem proof, with a consistent branch of .
For , the indicator function has Mellin transform
The interval stays away from both zero and infinity, so the integral is absolutely convergent for every complex number . Its Mellin fundamental strip is the whole complex plane. Evaluating the antiderivative proves the formula for ; at , integrating gives the real natural logarithm . The apparent division by zero is a removable singularity, since by the Taylor series of the exponential function. The transform is an entire function.
For example, gives with value at zero. On , the Mellin transform sums oscillations over the width of the interval in natural logarithm coordinates; this is the same cancellation mechanism as in the Fourier transform of an interval indicator.
The fundamental strip of a Mellin transform is the interior of the set of real parts for which
Viewed in the complex plane, it is a vertical strip ; either bound may be infinite, and the interior may be empty. Both endpoints of the improper integral must be checked. Convergence on a boundary line, whether absolute convergence or conditional convergence, requires a separate test. The Mellin transform is holomorphic throughout a nonempty fundamental strip.[ref]
A practical sufficient test uses Big O notation: if near zero and near infinity, with real , then comparison with elementary improper integrals gives
Thus guarantees absolute convergence. These upper bounds on need not locate the maximal Mellin fundamental strip; faster actual decay can widen it. The strip property itself follows by bounding the weight at any intermediate by the sum of two weights already known to be integrable. On a closed narrower strip, neighboring integrable weights also dominate the natural logarithm factors introduced by differentiation under the integral sign, making the transform a holomorphic function.
An exact two-endpoint example is
Here both bounds are sharp: at the zero-end absolute convergence test contains , and at the infinity-end test contains . The displayed rational function continues meromorphically outside the Mellin fundamental strip and has simple poles at and . Its other finite continued values outside the strip are values of a meromorphic continuation, not of a convergent defining integral. More general endpoint information leads to meromorphic continuation of a Mellin transform from an asymptotic expansion.
Figure 1.
Two endpoint conditions define the Mellin fundamental strip
. Left: the Mellin fundamental strip for below one and above one is . Crosses mark the two poles of the continued rational function, not whole lines of isolated singularities. Right: the formula and independently computed integrals agree on the real slice inside the strip. The curve is drawn only where the defining integral converges. Details.
For , let . Whenever the Mellin transform of is absolutely convergent,
The Mellin fundamental strip is unchanged: the corresponding integrals of absolute values differ by the finite positive factor . The change of variables gives , proving the rule. For , the transform's absolute value changes by , while the factor changes its phase. On the line , wherever absolute convergence holds, the transform's absolute value is preserved.
For the Mellin transform of an interval indicator, replacing by gives
At the removable singularity , both sides have value . Scaling leaves the width measured by the natural logarithm unchanged. Likewise, the exponential function has Mellin transform on .
Figure 1.
Scaling a positive variable translates its logarithmic coordinate
. Left: moves the support interval to . Right: turns the same change into a translation to the left by ; the interval width remains . The scaling property of the Mellin transform multiplies the transform by . Details.
The change of variables , using the exponential function, turns the Mellin transform into
The factor changes to ; missing this factor would shift every exponent by one. With and the Fourier transform convention , the identity is
Choosing inside the Mellin fundamental strip makes a Lebesgue integrable function. The minus sign in the Fourier transform argument follows from the stated convention. For the Mellin transform of an interval indicator with and , : the Fourier transform of an interval indicator is literally the same computation in a different coordinate.
Splitting the real line at also connects the Mellin transform to two unilateral Laplace transforms. If and for , then
where both integrals converge absolutely. Their Laplace convergence regions impose opposite endpoint conditions, explaining the two sides of the Mellin fundamental strip. Finally, shows that a change of scale is a translation in . Weighted Fourier transforms of this translation give exactly the factor in the scaling property of the Mellin transform. For a smooth function with compact support inside , the Mellin inversion theorem follows from Fourier inversion; the existing formula states the corresponding hypotheses.
Let and . Near zero, the complex integral fails both absolute and ordinary convergence through its real part, which behaves as . Taking the imaginary part first gives
The regularized integrand is integrable at zero: setting changes its tail to a function comparable to . Exponential decay controls infinity, and prevents an interior singularity at .
A family with positive Mellin transform exponent can consequently have a finite imaginary-part boundary limit even when its full complex limit does not exist. Taking the limit of the full divergent expression and only then selecting its imaginary part is not justified. Endpoint-expansion coefficients can also change nonuniformly: a sine zero may cancel a gamma function pole and leave a nonzero constant term. This explains the regularization needed in the logarithmic expansion of Ramanujan's function.
Let be a real random variable, and let be the undiscounted call value at log-strike , where . For and ,
For a fixed value of , only contributes. Direct integration gives
For real , Tonelli theorem allows interchange with expectation; for complex in the stated exponential moment domain, absolute integrability gives the same interchange. This expresses the moment-generating function of a log-price through a continuum of option prices. Discounting, forward normalization and a restricted strike range require corresponding adjustments.
Suppose decays faster than every power at infinity and, near zero, for every , with strictly increasing and tending to infinity. Subtracting finitely many terms in the integral over gives
The last integral is holomorphic on . These expressions continue the Mellin transform meromorphically to the whole plane, with simple poles precisely at for nonzero .
Strict increase alone does not suffice in the preceding theorem. Let , and , where is continuous, equals one on and vanishes on . After division by the next power, every finite remainder extends continuously to zero. Nevertheless the Mellin transform has genuine poles at accumulating at , so it cannot be a meromorphic function on the whole plane.
Under standard decay and regularity hypotheses,
If is smooth and compactly supported in , its Mellin transform is entire, decays faster than every power on vertical lines, and the formula holds for every real and every .
The unilateral Laplace transform of a function is the integral transform
Here is a complex number, is its real part, and is the imaginary unit. The exponential function factor weights the history, while probes its oscillations. The integral starts at zero, so it uses only the history from that starting time onward. This section concerns ordinary functions; their value at the single endpoint does not change the integral. See MIT 18.03SC, definition and elementary examples.
The Laplace transform is useful because it packages an entire time history into a function of : a derivative becomes multiplication by together with the initial value, and a convolution becomes a product. Thus a linear differential equation can become an algebraic equation that already remembers its initial value problem. The worked example below shows both descriptions of the same response.
If is a piecewise continuous function and has exponential order , then its defining integral is absolutely convergent for . This is a sufficient condition; the actual Laplace convergence region may be larger than the bound obtained from a chosen . [ref].
Figure 1. . Left: for , the weighted function decays when , stays at one when , and grows when . Right: the real-parameter Laplace transforms of and grow without bound as approaches their respective convergence boundaries from the right. Curves are drawn only where the defining integrals converge. Details.
The bound has a short explanation. For sufficiently large , , so , whose tail integral is finite for . The finite initial interval is covered by piecewise continuity.
Three calculations make the convergence condition concrete. For the input , evaluate the finite-history integral first:
At the finite-history integral is . For the exponential function input , the same calculation replaces by , giving
In particular, is allowed for this decaying input: its weighted integral is . For the sine input, Euler's formula gives ; linearity then yields
The Laplace convergence region is part of the answer. For example, has an analytic continuation to , but the defining integral for the input diverges there. The sine calculation is also developed in MIT 18.03SC, further elementary transforms.
To see why the initial value appears, suppose is an absolutely continuous function on every finite interval , with its right one-sided limit. At the chosen , assume and are Lebesgue integrable functions and . The Laplace transform of a derivative is then
For example, exponential order bounds on both and guarantee these conditions whenever exceeds both growth bounds. The initial value is the lower-end boundary contribution of integration by parts.
Consider the initial value problem
Write . The Laplace transform of a derivative and linearity give for . A partial fraction decomposition therefore gives
We recognize the two elementary Laplace transforms already computed. Directly verify the result: its derivative is , so
This verifies both the ordinary differential equation and the initial value, and shows that the resulting bounded function has the Laplace transform used above. The response rises from zero toward : at that value the input balances the term . The general method is described in MIT 18.03SC, solving initial value problems.
Figure 2.
A Heaviside step function input produces a response equal to the accumulated convolution kernel
. Left: the solution and the convolution kernel for . Right: at , the shaded integral includes only the available history . The rising profile on the right is ; recent inputs have had less time to decay. Details.
The same solution is a convolution. For functions defined on , the unilateral convolution is
The main convolution article integrates over the whole real line; applying a causal extension by zero to both functions makes its formula identical to this one. Nonzero contributions require both and , hence . If and are Lebesgue integrable functions on , the convolution theorem for Laplace transforms states
For piecewise continuous functions of exponential order and , it holds throughout . The weighted absolute double integral factors into the two finite weighted absolute integrals; Fubini's theorem therefore permits exchanging the order, and setting separates the product. [ref].
For the linear time-invariant system starting at zero, the convolution kernel is its impulse response for , extended by zero for . With the Heaviside step function input, for , the accumulated response is
Thus on is both the algebraic solution and the Laplace transform of a finite-history convolution. Each past input contributes an exponential function that decays with its age , which makes the two descriptions easy to connect.
Finally, compare the Fourier transform convention . If is the causal extension by zero of , define . Whenever is a Lebesgue integrable function,
A vertical slice of the Laplace transform is therefore the Fourier transform of the zero-extended, weighted input. Positive damps its positive-time history. A finite window function instead gives and ; this approaches in the Laplace convergence region. Setting directly requires an integrable zero-extended input: the input fails that condition, even though its Laplace transform exists for every .
The history of the Laplace transform spans several stages. Schiff's historical summary notes that Laplace's 1812 treatise acknowledged earlier work on integral transforms and describes later development of the modern Laplace transform method. [ref].
A bounded function on has a Laplace transform satisfying the displayed bound, by integration of . Consequently its Laplace transform cannot have a pole of order two or higher at . This can eliminate the arbitrary constant introduced when multiplication by turns an ordinary differential equation into a first-order differential equation for its Laplace transform.
For example, transforming with gives . An integrating factor yields
The bound forces , selecting . This selection can be justified without assuming unproved endpoint regularity for every solution: and have nonzero Wronskian on , so they form a fundamental system of solutions. Boundedness removes , and the limit at zero fixes the remaining coefficient. The endpoint limit by itself does not select a unique solution.
If two piecewise continuous functions of exponential order on have the same unilateral Laplace transform for every sufficiently large positive real parameter, they agree at every common point of continuity and agree almost everywhere. For continuous functions, the equality holds everywhere. Values at an isolated discontinuity cannot be recovered from an ordinary integral transform.
For real , the Laplace transform of the order-zero Bessel function of the first kind satisfies . This follows by transforming , using and , . Thus ; the initial value theorem for Laplace transforms gives and fixes .
For a function continuous at zero and of exponential order, the displayed limit recovers its initial value from its Laplace transform. Substitute to obtain and apply the dominated convergence theorem; an exponential-order bound controls the tail. The limit along positive real suffices for this version.
A function has exponential order if some and give the displayed bound. Bounded functions, including sine, have exponential order zero; has exponential order . The bound need not use the smallest possible . Together with piecewise continuity, it guarantees a Laplace transform for .
The set of complex numbers for which the displayed integral is finite is the region of absolute convergence of a Laplace transform. It depends only on the real part . Once the condition holds for one , it holds for every larger real part. For the exponential function it is exactly ; in general, convergence on the boundary must be checked separately. An analytic continuation outside this set need not equal a convergent defining integral.
Extend a function given for nonnegative time to the real line by setting it to zero before the starting time. This turns unilateral convolution into whole-line convolution and identifies a Laplace transform slice with a Fourier transform after exponential function weighting.
For , this Laplace transform converges at zero because is integrable, and at infinity because of exponential damping. Its large- behavior is governed by a logarithmic zero-endpoint singularity and begins with , rather than a power of .
The Gamma reflection formula gives , analytic at zero with value one. A finite-parameter Watson's lemma representation of Ramanujan's function therefore gives the displayed coefficients. In particular , and , with Euler's constant. Obtaining this representation requires taking an imaginary part before sending its Mellin exponent to zero; the original complex integral is divergent at that boundary.
For bounded locally integrable on the nonnegative real line, suppose its Laplace transform extends holomorphically to an open neighborhood of the closed right half-plane. Then the ordinary improper integral converges to . Contour damping for bounded Laplace transforms bounds the difference from the finite-interval transform by in the limit for every radius . Extension merely to the open right half-plane is insufficient, as the constant function and transform show.
The displayed kernel has residue one at zero and vanishes at the endpoints of a radius- imaginary-axis segment. On either radius- semicircle, , cancelling the inverse real-part bound on a bounded function's Laplace transform tail. Use the full transform only on a right semicircle and a thin analytic leftward path; deform the finite-interval entire transform to the large left semicircle. This proves the Newman Tauberian theorem without assuming analytic continuation across an entire left half-disk.
For functions on with and Lebesgue integrable functions, their unilateral convolution, defined almost everywhere if necessary, satisfies
Taking a causal extension by zero of both functions gives the existing whole-line convolution definition. Absolute convergence and Fubini's theorem justify the product rule: put in the double integral, so . For piecewise continuous functions of exponential order and , the hypotheses hold for . The Laplace transform article works out the concrete example and the Heaviside step function input, whose output is . [ref].
Let be of exponential order , piecewise continuously differentiable on finite intervals of nonnegative time, and let be its unilateral Laplace transform. For and at a point of continuity,
At a jump the symmetric integral recovers . The vertical line must lie in the defining region of absolute convergence of a Laplace transform; saying only that it avoids singularities of an analytic continuation does not supply that condition.[ref]
To see the inversion mechanism, extend by zero to negative time. Its Fourier transform at angular frequency is . The Fourier inversion theorem, followed by multiplication by and the substitution , gives the displayed formula. Contour deformation is a subsequent step that needs separate growth estimates.
A Laplace transform can grow exponentially as . At an evaluation time , multiplying by does not automatically permit closing the inverse contour to the left. Either retain the growth-bearing contour pieces, use a causal time convolution, or justify a deformation with the time-truncated transform. Resolvent-pole information alone is insufficient.
Terms singular at in a Laplace transform encode persistent late-time behaviour. In particular,
contributes to the inverse transform; singularities farther into the left half-plane contribute decaying terms under the usual analyticity and growth assumptions.
Suppose is an absolutely continuous function on every finite interval , both and are Lebesgue integrable functions, and . Then integration by parts on followed by a limit gives
Here is the right one-sided limit. Exponential order bounds on and suffice when exceeds both bounds. For , the identity reads on . This is the ordinary derivative on nonnegative time; differentiating a causal extension by zero at its jump instead introduces a Dirac delta function. [ref].
For , .
The delayed unit step has
The Heaviside step function switches from zero to one at its threshold. With threshold zero,
The value at zero is a convention, commonly zero, one half or one; changing this single value changes no ordinary integral. The delayed signal is zero before time and then follows the original signal from its beginning. This is the switch used by the Laplace transform shift theorem.
As a distribution, its derivative is the Dirac delta function: . Indeed, against a smooth compactly supported test function , one has . Ordinary pointwise differentiation away from zero would miss this concentrated jump.
Let , and let be a locally integrable function with period on nonnegative time. For , its unilateral Laplace transform is
Split the defining integral into successive periods and put . Periodicity makes each piece ; summing the absolutely convergent geometric series proves the formula. Local integrability on one period also controls the corresponding absolute integrals.
For a square pulse equal to one on and zero on , repeated periodically, the result is in that half-plane. At the defining improper integral generally fails; continuing the quotient algebraically does not enlarge the defining region of absolute convergence of a Laplace transform.
The Laplace transform of a matrix-valued function is obtained by transforming each entry. A constant matrix may be taken outside on the corresponding side of the integral; in particular, when is constant.
For a constant matrix and a forcing vector-valued function , consider
When the component Laplace transforms converge and the Laplace transform of a derivative applies, setting and gives
Choose in the convergence half-plane and outside the spectrum of . The resolvent is the Laplace transform of the matrix exponential for sufficiently large real part. Inverting gives the variation-of-constants formula
The matrix acts on the forcing from the left, so there is no implicit commutation of a time-dependent forcing with .

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