For example, in an oriented 3-dimensional Euclidean space, an oriented plane can be represented by the exterior product of two basis vectors, and its Hodge dual is the normal vector given by their cross product; conversely, any vector is dual to the oriented plane perpendicular to it, endowed with a suitable bivector. Generalizing this to an n-dimensional vector space, the Hodge star is a one-to-one mapping of k-vectors to (n – k)-vectors; the dimensions of these spaces are the binomial coefficients.
The Hodge star operator is a linear operator on the exterior algebra of V, mapping k-vectors to (n – k)-vectors, for . It has the following property, which defines it completely:: 15
for every pair of k-vectors
Dually, in the space of n-forms (alternating n-multilinear functions on ), the dual to is the volume form, the function whose value on is the determinant of the matrix assembled from the column vectors of in -coordinates.
Applying to the above equation, we obtain the dual definition:
or equivalently, taking , , and :
This means that, writing an orthonormal basis of k-vectors as over all subsets of , the Hodge dual is the (n – k)-vector corresponding to the complementary set :
The Hodge star is motivated by the correspondence between a subspace W of V and its orthogonal subspace (with respect to the inner product), where each space is endowed with an orientation and a numerical scaling factor. Specifically, a non-zero decomposable k-vector corresponds by the Plücker embedding to the subspace with oriented basis , endowed with a scaling factor equal to the k-dimensional volume of the parallelepiped spanned by this basis (equal to the Gramian, the determinant of the matrix of inner products ). The Hodge star acting on a decomposable vector can be written as a decomposable (n − k)-vector:
where form an oriented basis of the orthogonal space. Furthermore, the (n − k)-volume of the -parallelepiped must equal the k-volume of the -parallelepiped, and must form an oriented basis of V.
A general k-vector is a linear combination of decomposable k-vectors, and the definition of the Hodge star is extended to general k-vectors by defining it as being linear.
In two dimensions with the normalized Euclidean metric and orientation given by the ordering (x, y), the Hodge star on k-forms is given by
On the complex plane regarded as a real vector space with the standard sesquilinear form as the metric, the Hodge star has the remarkable property that it is invariant under holomorphic changes of coordinate. If z = x + iy is a holomorphic function of w = u + iv, then by the Cauchy–Riemann equations we have that ∂x/∂u = ∂y/∂v and ∂y/∂u = −∂x/∂v. In the new coordinates
A common example of the Hodge star operator is the case n = 3, when it can be taken as the correspondence between vectors and bivectors. Specifically, for EuclideanR3 with the basis of one-forms often used in vector calculus, one finds that
The Hodge star relates the exterior and cross product in three dimensions:
Applied to three dimensions, the Hodge star provides an isomorphism between axial vectors and bivectors, so each axial vector a is associated with a bivector A and vice versa, that is:.
The Hodge star can also be interpreted as a form of the geometric correspondence between an axis and an infinitesimal rotation around the axis, with speed equal to the length of the axis vector. An inner product on a vector space gives an isomorphism identifying with its dual space, and the space of all linear operators is naturally isomorphic to the tensor product. Thus for , the star mapping takes each vector to a bivector , which corresponds to a linear operator . Specifically, is a skew-symmetric operator, which corresponds to an infinitesimal rotation: that is, the macroscopic rotations around the axis are given by the matrix exponential. With respect to the basis of , the tensor corresponds to a coordinate matrix with 1 in the row and column, etc., and the wedge is the skew-symmetric matrix , etc. That is, we may interpret the star operator as:
Under this correspondence, cross product of vectors corresponds to the commutator Lie bracket of linear operators: .
In case , the Hodge star acts as an endomorphism of the second exterior power (i.e. it maps 2-forms to 2-forms, since 4 − 2 = 2). If the signature of the metric tensor is all positive, i.e. on a Riemannian manifold, then the Hodge star is an involution. If the signature is mixed, i.e., pseudo-Riemannian, then application twice will return the argument up to a sign – see § Duality below. This particular endomorphism property of 2-forms in four dimensions makes self-dual and anti-self-dual two-forms natural geometric objects to study. That is, one can describe the space of 2-forms in four dimensions with a basis that “diagonalizes” the Hodge star operation with eigenvalues (or , depending on the signature).
For concreteness, we discuss Hodge dual in Minkowski spacetime where with metric signature and coordinates . The volume form is oriented as . For one-forms,
Hodge dual for three- and four-forms can be easily deduced from the fact that, in the Lorentzian signature, for odd-rank forms and for even-rank forms. An easy rule to remember for these Hodge operations is that given a form , its Hodge dual may be obtained by writing the components not involved in in an order such that .[verification needed] An extra minus sign will enter only if contains . (For (+ - - -), one puts in a minus sign only if involves an odd number of the space-associated forms , and .)
Note that, the combinations
takes as the eigenvalue for Hodge dual, i.e.,
and hence deserve the name self-dual and anti-self-dual two-forms. Understanding the geometry, or kinematics, of Minkowski spacetime in self-dual and anti-self-dual sectors turns out to be insightful in both mathematical and physical perspectives, making contacts to the use of the two-spinor language in modern physics such as spinor-helicity formalism or twistor theory.
The combination of the operator and the exterior derivatived generates the classical operators grad, curl, and div on vector fields in three-dimensional Euclidean space. This works out as follows: d takes a 0-form (a function) to a 1-form, a 1-form to a 2-form, and a 2-form to a 3-form (and takes a 3-form to zero). For a 0-form , the first case written out in components gives:
The inner product identifies 1-forms with vector fields as , etc., so that becomes .
In the second case, a vector field corresponds to the 1-form , which has exterior derivative:
Applying the Hodge star gives the 1-form:
which becomes the vector field .
In the third case, again corresponds to . Applying Hodge star, exterior derivative, and Hodge star again:
One advantage of this expression is that the identity d2 = 0, which is true in all cases, has as special cases two other identities: 1) curl grad f = 0, and 2) div curl F = 0. In particular, Maxwell's equations take on a particularly simple and elegant form, when expressed in terms of the exterior derivative and the Hodge star. The expression (multiplied by an appropriate power of -1) is called the codifferential; it is defined in full generality, for any dimension, further in the article below.
One can also obtain the LaplacianΔ f = div grad f in terms of the above operations:
The Laplacian can also be seen as a special case of the more general Laplace–deRham operator where is the codifferential for -forms. Any function is a 0-form, and and so this reduces to the ordinary Laplacian. For the 1-form above, the codifferential is and after some plug and chug, one obtains the Laplacian acting on .
Applying the Hodge star twice leaves a k-vector unchanged except for its sign: for in an n-dimensional space V, one has
where s is the parity of the signature of the inner product on V, that is, the sign of the determinant of the matrix of the inner product with respect to any basis. For example, if n = 4 and the signature of the inner product is either (+ − − −) or (− + + +) then s = −1. For Riemannian manifolds (including Euclidean spaces), we always have s = 1.
The above identity implies that the inverse of can be given as
If n is odd then k(n − k) is even for any k, whereas if n is even then k(n − k) has the parity of k. Therefore:
For an n-dimensional oriented pseudo-Riemannian manifoldM, we apply the construction above to each cotangent space and its exterior powers , and hence to the differential k-forms, the global sections of the bundle. The Riemannian metric induces an inner product on at each point . We define the Hodge dual of a k-form, defining as the unique (n – k)-form satisfying
We compute in terms of tensor index notation with respect to a (not necessarily orthonormal) basis in a tangent space and its dual basis in , having the metric matrix and its inverse matrix . The Hodge dual of a decomposable k-form is:
Here is the Levi-Civita symbol with , and we implicitly take the sum over all values of the repeated indices . The factorial accounts for double counting, and is not present if the summation indices are restricted so that . The absolute value of the determinant is necessary since it may be negative, as for tangent spaces to Lorentzian manifolds.
An arbitrary differential form can be written as follows:
The factorial is again included to account for double counting when we allow non-increasing indices. We would like to define the dual of the component so that the Hodge dual of the form is given by
Using the above expression for the Hodge dual of , we find:
Although one can apply this expression to any tensor , the result is antisymmetric, since contraction with the completely anti-symmetric Levi-Civita symbol cancels all but the totally antisymmetric part of the tensor. It is thus equivalent to antisymmetrization followed by applying the Hodge star.
The codifferential is not an antiderivation on the exterior algebra, in contrast to the exterior derivative.
The codifferential is the adjoint of the exterior derivative with respect to the square-integrable inner product:
where is a (k + 1)-form and a k-form. This property is useful as it can be used to define the codifferential even when the manifold is non-orientable (and the Hodge star operator not defined). The identity can be proved from Stokes' theorem for smooth forms:
provided M has empty boundary, or or has zero boundary values. (The proper definition of the above requires specifying a topological vector space that is closed and complete on the space of smooth forms. The Sobolev space is conventionally used; it allows the convergent sequence of forms (as ) to be interchanged with the combined differential and integral operations, so that and likewise for sequences converging to .)
Since the differential satisfies , the codifferential has the corresponding property
The Hodge star sends harmonic forms to harmonic forms. As a consequence of Hodge theory, the de Rham cohomology is naturally isomorphic to the space of harmonic k-forms, and so the Hodge star induces an isomorphism of cohomology groups
^ abPertti Lounesto (2001). "§3.6 The Hodge dual". Clifford Algebras and Spinors, Volume 286 of London Mathematical Society Lecture Note Series (2nd ed.). Cambridge University Press. p. 39. ISBN0-521-00551-5.