The Full Wiki

Levi-Civita symbol: Wikis


Note: Many of our articles have direct quotes from sources you can cite, within the Wikipedia article! This article doesn't yet, but we're working on it! See more info or our list of citable articles.


From Wikipedia, the free encyclopedia

The Levi-Civita symbol, also called the permutation symbol, antisymmetric symbol, or alternating symbol, is a mathematical symbol used in particular in tensor calculus. It is named after the Italian mathematician and physicist Tullio Levi-Civita.



Visualization of the Levi-Civita symbol.

In three dimensions, the Levi-Civita symbol is defined as follows:

 \varepsilon_{ijk} = \begin{cases} +1 & \mbox{if } (i,j,k) \mbox{ is } (1,2,3), (3,1,2) \mbox{ or } (2,3,1), \ -1 & \mbox{if } (i,j,k) \mbox{ is } (1,3,2), (3,2,1) \mbox{ or } (2,1,3), \ 0 & \mbox{otherwise: }i=j \mbox{ or } j=k \mbox{ or } k=i, \end{cases}

i.e.  \varepsilon_{ijk} is 1 if (i, j, k) is an even permutation of (1,2,3), −1 if it is an odd permutation, and 0 if any index is repeated.

The formula for the three dimensional Levi-Civita symbol is:

 \varepsilon_{ijk} = \frac{\left( j-i \right)\left( k-i \right)\left( k-j \right)}{2} = \frac{\left( i-j \right)\left( j-k \right)\left( k-i \right)}{2}

The formula in four dimensions is:

 \varepsilon_{ijkl} = \frac{\left( j-i \right)\left( k-i \right)\left( l-i \right)\left( k-j \right)\left( l-j \right)\left( l-k \right)}{12} = \frac{\left( i-j \right)\left( i-k \right)\left( i-l \right)\left( j-k \right)\left( j-l \right)\left( k-l \right)}{12}
Visualization of the Levi-Civita-Symbol. Empty cube means 0, red is 1 and blue is -1.

For example, in linear algebra, the determinant of a 3×3 matrix A can be written

 \det A = \sum_{i=1}^3 \sum_{j=1}^3 \sum_{k=1}^3 \varepsilon_{ijk} a_{1i} a_{2j} a_{3k}

(and similarly for a square matrix of general size, see below)

and the cross product of two vectors can be written as a determinant:

 \mathbf{a \times b} = \begin{vmatrix} \mathbf{e_1} & \mathbf{e_2} & \mathbf{e_3} \ a_1 & a_2 & a_3 \ b_1 & b_2 & b_3 \ \end{vmatrix} = \sum_{i=1}^3 \sum_{j=1}^3 \sum_{k=1}^3 \varepsilon_{ijk} \mathbf{e_i} a_j b_k

or more simply:

 \mathbf{a \times b} = \mathbf{c},\ c_i = \sum_{j=1}^3 \sum_{k=1}^3 \varepsilon_{ijk} a_j b_k.

According to the Einstein notation, the summation symbols may be omitted.

The tensor whose components in an orthonormal basis are given by the Levi-Civita symbol (a tensor of covariant rank n) is sometimes called the permutation tensor. It is actually a pseudotensor because under an orthogonal transformation of jacobian determinant −1 (i.e., a rotation composed with a reflection), it acquires a minus sign. Because the Levi-Civita symbol is a pseudotensor, the result of taking a cross product is a pseudovector, not a vector.

Note that under a general coordinate change, the components of the permutation tensor get multiplied by the jacobian of the transformation matrix. This implies that in coordinate frames different from the one in which the tensor was defined, its components can differ from those of the Levi-Civita symbol by an overall factor. If the frame is orthonormal, the factor will be ±1 depending on whether the orientation of the frame is the same or not.


Relation to Kronecker delta

The Levi-Civita symbol is related to the Kronecker delta. In three dimensions, the relationship is given by the following equations:

 \varepsilon_{ijk}\varepsilon_{lmn} = \det \begin{bmatrix} \delta_{il} & \delta_{im}& \delta_{in}\ \delta_{jl} & \delta_{jm}& \delta_{jn}\ \delta_{kl} & \delta_{km}& \delta_{kn}\ \end{bmatrix}
 = \delta_{il}\left( \delta_{jm}\delta_{kn} - \delta_{jn}\delta_{km}\right) - \delta_{im}\left( \delta_{jl}\delta_{kn} - \delta_{jn}\delta_{kl} \right) + \delta_{in} \left( \delta_{jl}\delta_{km} - \delta_{jm}\delta_{kl} \right) \,
 \sum_{i=1}^3 \varepsilon_{ijk}\varepsilon_{imn} = \delta_{jm}\delta_{kn} - \delta_{jn}\delta_{km} ("contracted epsilon identity")

(In Einstein notation, the duplication of the i index implies the sum on i. The previous is then noted:  \varepsilon_{ijk}\varepsilon_{imn} = \delta_{jm}\delta_{kn} - \delta_{jn}\delta_{km})

 \sum_{i=1}^3 \sum_{j=1}^3 \varepsilon_{ijk}\varepsilon_{ijn} = 2\delta_{kn}

Generalization to n dimensions

The Levi-Civita symbol can be generalized to higher dimensions:

\varepsilon_{ijkl\dots} = \begin{cases} +1 & \mbox{if }(i,j,k,l,\dots) \mbox{ is an even permutation of } (1,2,3,4,\dots) \ -1 & \mbox{if }(i,j,k,l,\dots) \mbox{ is an odd permutation of } (1,2,3,4,\dots) \ 0 & \mbox{if any two labels are the same} \end{cases}

Thus, it is the sign of the permutation in the case of a permutation, and zero otherwise.

The generalized formula is:

 \varepsilon_{a_1 a_2 a_3 \ldots a_n} = \prod_{i=1}^{n-1} \left( \frac{1}{i!} \ \prod_{j=i+1}^n ( a_j-a_i ) \right)

where n is the dimension (rank).

For any n the property

 \sum_{i,j,k,\dots=1}^n \varepsilon_{ijk\dots}\varepsilon_{ijk\dots} = n!

follows from the facts that (a) every permutation is either even or odd, (b) (+1)2 = (-1)2 = 1, and (c) the permutations of any n-element set number exactly n!.

In index-free tensor notation, the Levi-Civita symbol is replaced by the concept of the Hodge dual.

In general n dimensions one can write the product of two Levi-Civita symbols as:

 \varepsilon_{i_1 i_2 \dots i_n} \varepsilon_{j_1 j_2 \dots j_n} = \det \begin{bmatrix} \delta_{i_1 j_1} & \delta_{i_1 j_2} & \dots & \delta_{i_1 j_n} \ \delta_{i_2 j_1} & \delta_{i_2 j_2} & \dots & \delta_{i_2 j_n} \ \vdots & \vdots & \vdots & \vdots \ \delta_{i_n j_1} & \delta_{i_n j_2} & \dots & \delta_{i_n j_n} \ \end{bmatrix} .


(in these examples, superscripts should be considered equivalent with subscripts)

1. In two dimensions, when all i,j,m,n are in {1,2},

 \varepsilon_{ij} \varepsilon^{mn} =  \delta_i^m \delta_j^n - \delta_i^n \delta_j^m, (1)
 \varepsilon_{ij} \varepsilon^{in} =  \delta_j^n, (2)
 \varepsilon_{ij} \varepsilon^{ij}=2. (3)

2. In three dimensions, when all i,j,k,m,n are in {1,2,3},

 \varepsilon_{jmn} \varepsilon^{imn}=2\delta^i_j, (4)
 \varepsilon_{ijk} \varepsilon^{ijk}=6, (5)
 \varepsilon_{ijk} \varepsilon^{imn}=\delta^{m}_j\delta^{n}_k - \delta^{n}_j\delta^{m}_k. (6)

3. In n dimensions, when all i1,...,in,j1,...,jn are in {1,...,n},:

 \varepsilon_{i_1...i_n} \varepsilon^{j_1...j_n} = n! \delta^{j_1}_{[i_1}...\delta^{j_n}_{i_n]}, (7)
 \varepsilon_{i_1...i_k i_{k+1}...i_n} \varepsilon^{i_1...i_k j_{k+1}...j_n} = k! (n-k)! \delta^{j_{k+1}}_{[i_{k+1}}...\delta^{j_n}_{i_n]}, (8)
 \varepsilon_{i_1...i_n} \varepsilon^{i_1...i_n} = n!. (9)


For equation 1, both sides are antisymmetric with respect of ij and mn. We therefore only need to consider the case i\neq j and m\neq n. By substitution, we see that the equation holds for \varepsilon_{12} \varepsilon^{12}, i.e., for i = m = 1 and j = n = 2. (Both sides are then one). Since the equation is antisymmetric in ij and mn, any set of values for these can be reduced to the above case (which holds). The equation thus holds for all values of ij and mn. Using equation 1, we have for equation 2  \varepsilon_{ij}\varepsilon^{in} =  \delta_i^i \delta_j^n - \delta^n_i \delta^i_j

=  2 \delta_j^n - \delta^n_j
=  \delta_j^n.

Here we used the Einstein summation convention with i going from 1 to 2. Equation 3 follows similarly from equation 2. To establish equation 4, let us first observe that both sides vanish when i\neq j. Indeed, if i\neq j, then one can not choose m and n such that both permutation symbols on the left are nonzero. Then, with i = j fixed, there are only two ways to choose m and n from the remaining two indices. For any such indices, we have \varepsilon_{jmn} \varepsilon^{imn} = (\varepsilon^{imn})^2 = 1 (no summation), and the result follows. Property (5) follows since 3! = 6 and for any distinct indices i,j,k in {1,2,3}, we have \varepsilon_{ijk} \varepsilon^{ijk}=1 (no summation).


1. The determinant of an n\times n matrix A = (aij) can be written as

 \det A = \varepsilon_{i_1\cdots i_n} a_{1i_1} \cdots a_{ni_n},

where each il should be summed over 1,\ldots, n.

Equivalently, it may be written as

 \det A = \frac{1}{n!} \varepsilon_{i_1\cdots i_n} \varepsilon_{j_1\cdots j_n} a_{i_1 j_1} \cdots a_{i_n j_n},

where now each il and each jl should be summed over 1,\ldots, n.

2. If A = (A1,A2,A3) and B = (B1,B2,B3) are vectors in R3 (represented in some right hand oriented orthonormal basis), then the ith component of their cross product equals

 (A\times B)^i = \varepsilon^{ijk} A^j B^k.

For instance, the first component of A\times B is A2B3A3B2. From the above expression for the cross product, it is clear that A\times B = -B\times A. Further, if C = (C1,C2,C3) is a vector like A and B, then the triple scalar product equals

 A\cdot(B\times C) = \varepsilon^{ijk} A^i B^j C^k.

From this expression, it can be seen that the triple scalar product is antisymmetric when exchanging any adjacent arguments. For example, A\cdot(B\times C)= -B\cdot(A\times C).

3. Suppose F = (F1,F2,F3) is a vector field defined on some open set of R3 with Cartesian coordinates x = (x1,x2,x3). Then the ith component of the curl of F equals

 (\nabla \times F)^i(x) = \varepsilon^{ijk}\frac{\partial}{\partial x^j} F^k(x).


A shorthand notation for anti-symmetrization is denoted by a pair of square brackets. For example, in arbitrary dimensions, for a rank 2 covariant tensor M,

M_{[ab]} = \frac{1}{2!}(M_{ab} - M_{ba}) \,,

and for a rank 3 covariant tensor T,

T_{[abc]} = \frac{1}{3!}(T_{abc}-T_{acb}+T_{bca}-T_{bac}+T_{cab}-T_{cba}) \,.

In three dimensions, these are equivalent to

M_{[ab]} = \varepsilon_{abc} \, \frac{1}{2!} \, \varepsilon^{dec} M_{de} \,,
T_{[abc]} = \varepsilon_{abc} \, \frac{1}{3!} \, \varepsilon^{def} T_{def} \,.

While in four dimensions, these are equivalent to

M_{[ab]} = \frac{1}{2!} \, \varepsilon_{abcd} \, \frac{1}{2!} \, \varepsilon^{efcd} M_{ef} \,,
T_{[abc]} = \varepsilon_{abcd} \, \frac{1}{3!} \, \varepsilon^{efgd} T_{efg} \,.

Tensor density

The Levi-Civita symbol may be considered to be a tensor density in two different ways. It may be regarded as a contravariant tensor density of weight +1 or as a covariant tensor density of weight -1. In four dimensions,

\epsilon^{\alpha \beta \gamma \delta} = -\epsilon_{\alpha \beta \gamma \delta} \,.

See also


This article incorporates material from Levi-Civita permutation symbol on PlanetMath, which is licensed under the Creative Commons Attribution/Share-Alike License.


Got something to say? Make a comment.
Your name
Your email address