In mathematics, a radial function is a real-valued function defined on a Euclidean space Rn whose value at each point depends only on the distance between that point and the origin. The distance is usually the Euclidean distance. For example, a radial function Φ in two dimensions has the form[1]
\Phi(x,y)=\varphi(r), r=\sqrt{x2+y2}
A function is radial if and only if it is invariant under all rotations leaving the origin fixed. That is, ƒ is radial if and only if
f\circ\rho=f
S[\varphi]=S[\varphi\circ\rho]
Given any (locally integrable) function ƒ, its radial part is given by averaging over spheres centered at the origin. To wit,
\phi(x)=
1 | |
\omegan-1 |
\int | |
Sn-1 |
f(rx')dx'
The Fourier transform of a radial function is also radial, and so radial functions play a vital role in Fourier analysis. Furthermore, the Fourier transform of a radial function typically has stronger decay behavior at infinity than non-radial functions: for radial functions bounded in a neighborhood of the origin, the Fourier transform decays faster than R-(n-1)/2. The Bessel functions are a special class of radial function that arise naturally in Fourier analysis as the radial eigenfunctions of the Laplacian; as such they appear naturally as the radial portion of the Fourier transform.