In mathematics, the Kronecker delta or Kronecker's delta, named after Leopold Kronecker, is a function of two variables, usually just positive integers. The function is 1 if the variables are equal, and 0 otherwise:

\delta_{ij} = \begin{cases} 0 &\text{if } i \neq j, \\ 1 &\text{if } i=j. \end{cases}
where the Kronecker delta δ_{ij} is a piecewise function of variables i and j. For example, δ_{1 2} = 0, whereas δ_{3 3} = 1.
The Kronecker delta appears naturally in many areas of mathematics, physics and engineering, as a means of compactly expressing its definition above.
In linear algebra, the n × n identity matrix I has entries equal to the Kronecker delta:

\left( I \right)_{ij} = \delta_{ij} \,
where i and j take the values 1, 2, ..., n, and the inner product of vectors can be written as

\textstyle \boldsymbol{a}\cdot\boldsymbol{b} = \sum_{ij} a_{i}\delta_{ij}b_{j}.
The restriction to positive integers is common, but there is no reason it cannot have negative integers as well as positive, or any discrete rational numbers. If i and j above take rational values, then for example δ_{−1, −3} = 0 and δ_{+1/2, −3/2} = 0 but δ_{−2,−2} = 1 and δ_{5/3, 5/3} = 1. This latter case is ultimately for convenience.
Contents

Properties 1

Alternative notation 2

Digital signal processing 3

Properties of the delta function 4

Relationship to the Dirac delta function 5

Generalizations of the Kronecker delta 6

Definitions of generalized Kronecker delta 6.1

Properties of generalized Kronecker delta 6.2

Integral representations 7

The Kronecker comb 8

Kronecker integral 9

See also 10

References 11
Properties
The following equations are satisfied:

\begin{align} \sum_{j} \delta_{ij} a_j &= a_i,\\ \sum_{i} a_i\delta_{ij} &= a_j,\\ \sum_{k} \delta_{ik}\delta_{kj} &= \delta_{ij}. \end{align}
Therefore, δ_{ij} can be considered as an identity matrix.
Alternative notation
Using the Iverson bracket:

\delta_{ij} = [i=j ].\,
Often, the notation \delta_i is used.

\delta_{i} = \begin{cases} 0, & \mbox{if } i \ne 0 \\ 1, & \mbox{if } i=0 \end{cases}
In linear algebra, it can be thought of as a tensor, and is written \delta^i_j. Sometimes the Kronecker delta is called the substitution tensor.^{[1]}
Digital signal processing
An impulse function
Similarly, in digital signal processing, the same concept is represented as a sequence or discrete function on \mathbb{Z} (the integers):

\delta[n] = \begin{cases} 0, & n \ne 0 \\ 1, & n = 0.\end{cases}
The function is referred to as an impulse, or unit impulse. When it is the input to a discretetime signal processing element, the output is called the impulse response of the element.
Properties of the delta function
The Kronecker delta has the socalled sifting property that for j\in\mathbb Z:

\sum_{i=\infty}^\infty a_i \delta_{ij} =a_j.
and if the integers are viewed as a measure space, endowed with the counting measure, then this property coincides with the defining property of the Dirac delta function

\int_{\infty}^\infty \delta(xy)f(x) dx=f(y),
and in fact Dirac's delta was named after the Kronecker delta because of this analogous property. In signal processing it is usually the context (discrete or continuous time) that distinguishes the Kronecker and Dirac "functions". And by convention, \delta(t)\, generally indicates continuous time (Dirac), whereas arguments like i, j, k, l, m, and n are usually reserved for discrete time (Kronecker). Another common practice is to represent discrete sequences with square brackets; thus: \delta[n]\,. It is important to note that the Kronecker delta is not the result of directly sampling the Dirac delta function.
The Kronecker delta forms the multiplicative identity element of an incidence algebra.^{[2]}
Relationship to the Dirac delta function
In probability theory and statistics, the Kronecker delta and Dirac delta function can both be used to represent a discrete distribution. If the support of a distribution consists of points \mathbf{x} = \{x_1,\dots,x_n\}, with corresponding probabilities p_1,\dots,p_n\,, then the probability mass function p(x)\, of the distribution over \mathbf{x} can be written, using the Kronecker delta, as

p(x) = \sum_{i=1}^n p_i \delta_{x x_i}.
Equivalently, the probability density function f(x)\, of the distribution can be written using the Dirac delta function as

f(x) = \sum_{i=1}^n p_i \delta(xx_i).
Under certain conditions, the Kronecker delta can arise from sampling a Dirac delta function. For example, if a Dirac delta impulse occurs exactly at a sampling point and is ideally lowpassfiltered (with cutoff at the critical frequency) per the Nyquist–Shannon sampling theorem, the resulting discretetime signal will be a Kronecker delta function.
Generalizations of the Kronecker delta
If it is considered as a type (1,1) tensor, the Kronecker tensor, it can be written \delta^i_j with a covariant index j and contravariant index i:

\delta^{i}_{j} = \begin{cases} 0 & (i \ne j), \\ 1 & (i = j). \end{cases}
This (1,1) tensor represents:

The identity mapping (or identity matrix), considered as a linear mapping V \to V or V^* \to V^*

The trace or tensor contraction, considered as a mapping V^* \otimes V \to K

The map K \to V^* \otimes V, representing scalar multiplication as a sum of outer products.
The generalized Kronecker delta of order 2p is a type (p,p) tensor that is a completely antisymmetric in its p upper indices, and also in its p lower indices.
Two definitions that differ by a factor of p! are in use. Below, the version is presented has nonzero components scaled to be ±1. The second version has nonzero components that are ±1/p!, which results in the explicit scaling factors in § Properties of generalized Kronecker delta below disappearing.^{[3]}
Definitions of generalized Kronecker delta
In terms of the indices:^{[4]}^{[5]}

\delta^{\mu_1 \dots \mu_p }_{\nu_1 \dots \nu_p} = \begin{cases} +1 & \quad \text{if } \nu_1 \dots \nu_p \text{ are distinct integers and are an even permutation of } \mu_1 \dots \mu_p \\ 1 & \quad \text{if } \nu_1 \dots \nu_p \text{ are distinct integers and are an odd permutation of } \mu_1 \dots \mu_p \\ \;\;0 & \quad \text{in all other cases}.\end{cases}
Let \mathfrak{S}_p be the symmetric group of degree p, then:

\delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} = \sum_{\sigma \in \mathfrak{S}_p} \sgn(\sigma)\, \delta^{\mu_1}_{\nu_{\sigma(1)}}\cdots\delta^{\mu_p}_{\nu_{\sigma(p)}} = \sum_{\sigma \in \mathfrak{S}_p} \sgn(\sigma)\, \delta^{\mu_{\sigma(1)}}_{\nu_1}\cdots\delta^{\mu_{\sigma(p)}}_{\nu_p}.
Using antisymmetrization:

\delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} = p! \delta^{\mu_1}_{\lbrack \nu_1} \dots \delta^{\mu_p}_{\nu_p \rbrack} = p! \delta^{\lbrack \mu_1}_{\nu_1} \dots \delta^{\mu_p \rbrack}_{\nu_p}.
In terms of a p × p determinant:^{[6]}

\delta^{\mu_1 \dots \mu_p }_{\nu_1 \dots \nu_p} = \begin{vmatrix} \delta^{\mu_1}_{\nu_1} & \cdots & \delta^{\mu_1}_{\nu_p} \\ \vdots & \ddots & \vdots \\ \delta^{\mu_p}_{\nu_1} & \cdots & \delta^{\mu_p}_{\nu_p} \end{vmatrix}.
Using the Laplace expansion (Laplace's formula) of determinant, it may be defined recursively:^{[7]}

\begin{align} \delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} & = \sum_{k=1}^p (1)^{p+k} \delta^{\mu_p}_{\nu_k} \delta^{\mu_1 \dots \mu_{k} \dots \check\mu_p}_{\nu_1 \dots \check\nu_k \dots \nu_{p}} \\ & = \delta^{\mu_p}_{\nu_p} \delta^{\mu_1 \dots \mu_{p1}}_{\nu_1 \dots \nu_{p1}}  \sum_{k=1}^{p1} \delta^{\mu_p}_{\nu_k} \delta^{\mu_1 \dots \mu_{k1} \; \mu_k \; \mu_{k+1} \dots \mu_{p1}}_{\nu_1 \dots \;\nu_{k1} \; \nu_p \; \nu_{k+1}\; \dots \nu_{p1}},\end{align}
where \check{~} indicates an index that is omitted from the sequence.
When p = n (the dimension of the vector space), in terms of the LeviCivita symbol:

\delta^{\mu_1 \dots \mu_n}_{\nu_1 \dots \nu_n} = \varepsilon^{\mu_1 \dots \mu_n}\varepsilon_{\nu_1 \dots \nu_n}.
Properties of generalized Kronecker delta
The generalized Kronecker delta may be used for antisymmetrization:

\frac{1}{p!} \delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} a^{\nu_1 \dots \nu_p} = a^{\lbrack \mu_1 \dots \mu_p \rbrack} ,

\frac{1}{p!} \delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} a_{\mu_1 \dots \mu_p} = a_{\lbrack \nu_1 \dots \nu_p \rbrack} .
From the above equations and the properties of antisymmetric tensor, we can derive the properties of the generalized Kronecker delta:

\frac{1}{p!} \delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} a^{\lbrack \nu_1 \dots \nu_p \rbrack} = a^{\lbrack \mu_1 \dots \mu_p \rbrack} ,

\frac{1}{p!} \delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} a_{\lbrack \mu_1 \dots \mu_p \rbrack} = a_{\lbrack \nu_1 \dots \nu_p \rbrack} ,

\frac{1}{p!} \delta^{\mu_1 \dots \mu_p}_{\nu_1 \dots \nu_p} \delta^{\nu_1 \dots \nu_p}_{\rho_1 \dots \rho_p} = \delta^{\mu_1 \dots \mu_p}_{\rho_1 \dots \rho_p} ,
which are the generalized version of formulae written in the section Properties. The last formula is equivalent to the Cauchy–Binet formula.
Reducing the order via summation of the indices may be expressed by the identity^{[8]}

\delta^{\mu_1 \dots \mu_s \, \mu_{s+1} \dots \mu_p}_{\nu_1 \dots \nu_s \, \mu_{s+1} \dots \mu_p} = \tfrac{(ns)!}{(np)!} \delta^{\mu_1 \dots \mu_s}_{\nu_1 \dots \nu_s}.
Using both the summation rule for the case p = n and the relation with the LeviCivita symbol, the summation rule of the LeviCivita symbol is derived:

\delta^{\mu_1 \dots \mu_s}_{\nu_1 \dots \nu_s} = {1 \over (ns)!}\, \varepsilon^{\mu_1 \dots \mu_s \, \rho_{s+1} \dots \rho_n}\varepsilon_{\nu_1 \dots \nu_s \, \rho_{s+1} \dots \rho_n}.
Integral representations
For any integer n, using a standard residue calculation we can write an integral representation for the Kronecker delta as the integral below, where the contour of the integral goes counterclockwise around zero. This representation is also equivalent to a definite integral by a rotation in the complex plane.

\delta_{x,n} = \frac1{2\pi i} \oint_{z=1} z^{xn1} dz=\frac1{2\pi} \int_0^{2\pi} e^{i(xn)\varphi} d\varphi
The Kronecker comb
The Kronecker comb function with period N is defined (using DSP notation) as:

\Delta_N[n]=\sum_{k=\infty}^\infty \delta[nkN],
where N and n are integers. The Kronecker comb thus consists of an infinite series of unit impulses N units apart, and includes the unit impulse at zero. It may be considered to be the discrete analog of the Dirac comb.
Kronecker integral^{[9]}
The Kronecker delta is also called degree of mapping of one surface into another. Suppose a mapping takes place from surface S_{uvw} to S_{xyz} that are boundaries of regions, R_{uvw} and R_{xyz} which is simply connected with onetoone correspondence. In this framework, if s and t are parameters for S_{uvw} , and S_{uvw} to S_{xyz} are each oriented by the outer normal n:

u=u(s,t), v=v(s,t),w=w(s,t),
while the normal has the direction of:

(u_{s} i +v_{s} j + w_{s} k) \times (u_{t}i +v_{t}j +w_{t}k).
Let x=x(u,v,w),y=y(u,v,w),z=z(u,v,w) be defined and smooth in a domain containing S_{uvw}, and let these equations define the mapping of S_{uvw} into S_{xyz}. Then the degree \delta of mapping is 1/4\pi times the solid angle of the image S of S_{uvw} with respect to the interior point of S_{xyz}, O. If O is the origin of the region, R_{xyz}, then the degree, \delta is given by the integral:

\delta=\frac{1}{4\pi}\iint_{R_{st}}\frac{\begin{vmatrix}x&y&z\\\dfrac{\partial x}{\partial s}&\dfrac{\partial y}{\partial s}&\dfrac{\partial z}{\partial s}\\\dfrac{\partial x}{\partial t}&\dfrac{\partial y}{\partial t}&\dfrac{\partial z}{\partial t}\end{vmatrix}}{(x^2+y^2+z^2)\sqrt{x^2+y^2+z^2}}dsdt.
See also
References

^ Trowbridge, 1998. Journal of Atmospheric and Oceanic Technology. V15, 1 p291

^ Spiegel, Eugene; O'Donnell, Christopher J. (1997), Incidence algebras, Pure and Applied Mathematics 206, Marcel Dekker, .

^ http://people.physics.tamu.edu/pope/geomgroup.pdf Christopher Pope (2008), Geometry and Group Theory

^ Theodore Frankel, The Geometry of Physics: An Introduction 3rd edition (2012), published by Cambridge University Press, ISBN 9781107602601

^ D. C. Agarwal, Tensor Calculus and Riemannian Geometry 22nd edition (2007), published by Krishna Prakashan Media

^ David Lovelock, Hanno Rund (1989). Tensors, Differential Forms, and Variational Principles. Courier Dover Publications.

^ A recursive definition requires a first case, which may be taken as δ = 1 for p = 0, or alternatively δμ
ν = δμ
ν for p = 1 (generalized delta in terms of standard delta).

^ Sadri Hassani (2008). Mathematical Methods: For Students of Physics and Related Fields 2nd edition. SpringerVerlag.

^ Kaplan, Wilfred (2003), Advanced Calculus, Pearson Education. Inc, p. 364,
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