in n-dimensional Euclidean space is the convex body such that for any vector
in the direction u is the (n – 1)-dimensional volume of the projection of K onto the hyperplane orthogonal to u. Hermann Minkowski showed that the projection body of a convex body is convex.
Petty (1967) and Schneider (1967) used projection bodies in their solution to Shephard's problem.
There are two remarkable affine isoperimetric inequality for this body.
is n-dimensional volume, and there is equality precisely for ellipsoids.
The intersection body IK of K is defined similarly, as the star body such that for any vector u the radial function of IK from the origin in direction u is the (n – 1)-dimensional volume of the intersection of K with the hyperplane u⊥.
Equivalently, the radial function of the intersection body IK is the Funk transform of the radial function of K. Intersection bodies were introduced by Lutwak (1988).
Koldobsky (1998a) showed that a centrally symmetric star-shaped body is an intersection body if and only if the function 1/||x|| is a positive definite distribution, where ||x|| is the homogeneous function of degree 1 that is 1 on the boundary of the body, and Koldobsky (1998b) used this to show that the unit balls lpn, 2 < p ≤ ∞ in n-dimensional space with the lp norm are intersection bodies for n=4 but are not intersection bodies for n ≥ 5.