The delta function is a generalized function that can be defined as the limit of a class of delta sequences. The delta function is sometimes called "Dirac's delta function" or the "impulse symbol" (Bracewell 2000). It is implemented in the Wolfram Language as DiracDelta[x].
Formally,
is a linear functional from a space (commonly
taken as a Schwartz space
or the space of all smooth
functions of compact support
) of test functions
. The action of
on
, commonly denoted
or
, then gives the value at 0 of
for any test function
. In engineering contexts, the functional nature of the delta
function is often suppressed.
The limits of delta sequences are understood in the sense of generalized functions.
Their integrals against each smooth
function
of compact support converge to
. Pointwise convergence
of the defining functions is not required.
The delta function can be viewed as the derivative of the Heaviside step function,
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(1)
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(Bracewell 2000, p. 94).
The delta function has the fundamental property that
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(2)
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and, in fact,
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(3)
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for .
Additional identities include
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(4)
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for ,
as well as
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(5)
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(6)
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More generally, the delta function of a function of is given by
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(7)
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where the s
are the roots of
. For example, examine
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(8)
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Then ,
so
and
,
giving
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(9)
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The fundamental equation that defines derivatives of the delta function
is
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(10)
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Letting
in this definition, it follows that
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(11)
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(12)
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(13)
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where the second term can be dropped since , so (13) implies
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(14)
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In general, the same procedure gives
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(15)
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but since any power of times
integrates to 0, it follows that only the constant
term contributes. Therefore, all terms multiplied by derivatives
of
vanish, leaving
,
so
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(16)
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which implies
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(17)
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Other identities involving the derivative of the delta function include
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(18)
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(19)
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(20)
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where
denotes convolution,
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(21)
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and
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(22)
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An integral identity involving is given by
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(23)
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The delta function also obeys the so-called sifting property
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(24)
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(Bracewell 2000, pp. 74-75).
For ,
a Fourier series expansion of
on
gives
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(25)
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(26)
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(27)
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(28)
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so
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(29)
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(30)
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On the entire real line, this Fourier series represents the periodic impulse train , a shifted and rescaled
Shah function.
With the negative-exponent convention for the Fourier transform, the delta function is given by
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(31)
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The corresponding inverse Fourier transform gives
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(32)
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(Bracewell 2000, p. 95). More generally, the Fourier transform of the delta function is
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(33)
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The delta function has the following representations as limits of generalized functions as ,
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(34)
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(35)
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(36)
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(37)
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(38)
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(39)
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(40)
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where
is an Airy function,
is a Bessel
function of the first kind, and
is a Laguerre polynomial
of fixed polynomial degree
, with
a positive integer. The
Bessel function of the first kind
representation applies on
. The Laguerre polynomial
representation requires a normalization depending on
(R. Scholz, pers. comm., Feb. 9, 2017). The normalization
constant is
|
(41)
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For ,
substituting
shows that the Laguerre polynomial approximant
has unit integral and converges to the delta function
as
.
On ,
the delta function is also the distributional limit of
a normalized Dirichlet kernel as
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(42)
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On the entire real line, this limit is the periodic impulse train , a rescaled Shah
function.
Delta functions can also be defined in two dimensions, so that in two-dimensional Cartesian coordinates
|
(43)
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(44)
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(45)
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and
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(46)
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Similarly, in polar coordinates,
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(47)
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(Bracewell 2000, p. 89).
In three-dimensional Cartesian coordinates
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(48)
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(49)
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and
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(50)
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(51)
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(52)
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(Bracewell 2000, p. 90).
These formulas in polar coordinates, cylindrical coordinates, and spherical coordinates
use
and interpret
through symmetric delta sequences. In this convention,
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(53)
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The factors above give unit normalization when combined with the corresponding volume element. Alternatively, define a unit-normalized
radial delta function
by
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(54)
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The equivalent formulas are then
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(55)
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(56)
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(57)
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The radial normalization convention must therefore be specified when comparing these formulas (Gsponer 2007).
A series expansion in cylindrical coordinates gives
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(58)
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(59)
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The solution to some ordinary differential equations can be given in terms of derivatives
of
(Kanwal 1998). For example, the ordinary
differential equation
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(60)
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has classical solution
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(61)
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and distributional solution
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(62)
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(M. Trott, pers. comm., Jan. 19, 2006). Note that unlike classical solutions, a distributional solution to an th-order ODE need not contain
independent constants.