Orbital integral
In mathematics, an orbital integral is an integral transform that generalizes the spherical mean operator to homogeneous spaces. Instead of integrating over spheres, one integrates over generalized spheres: for a homogeneous space X = G/''H, a generalized sphere centered at a point x''0 is an orbit of the isotropy group of x0.
Definition
The model case for orbital integrals is a Riemannian symmetric space G/''K, where G'' is a Lie group and K is a symmetric compact subgroup. Generalized spheres are then actual geodesic spheres and the spherical averaging operator is defined aswhere
- the dot denotes the action of the group G on the homogeneous space Xg ∈ G is a group element such that x = g·''oy'' ∈ X is an arbitrary element of the geodesic sphere of radius r centered at x: d = r
- the integration is taken with respect to the Haar measure on K.
is the orbital integral centered at x over the orbit through y. As above, g is a group element that represents the coset x.
Integral geometry
A central problem of integral geometry is to reconstruct a function from knowledge of its orbital integrals. The Funk transform and Radon transform are two special cases. When G/''K is a Riemannian symmetric space, the problem is trivial, since M''rƒ is the average value of ƒ over the generalized sphere of radius r, andWhen K is compact, a similar shortcut works. The problem is more interesting when K is non-compact. For example, the Radon transform is the orbital integral that results by taking G to be the Euclidean isometry group and K the isotropy group of a hyperplane.
Orbital integrals are an important technical tool in the theory of automorphic forms, where they enter into the formulation of various trace formulas.