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We derive a formula connecting the derivatives of parallel section functions of an origin-symmetric star body in Rn with the Fourier transform of powers of the radial function of the body. A parallel section function (or (n - 1)-dimensional X-ray) gives the ((n - 1)-dimensional) volumes of all hyperplane sections of the body orthogonal to a given direction. This formula provides a new characterization of intersection bodies in Rn and leads to a unified analytic solution to the Busemann-Petty problem: Suppose that K and L are two origin-symmetric convex bodies in Rn such that the ((n - 1)-dimensional) volume of each central hyperplane section of K is smaller than the volume of; the corresponding section of L; is the (n-dimensional) volume of K smaller than the volume of L? In conjunction with earlier established connections between the Busemann-Petty problem, intersection bodies, and positive definite distributions, our formula shows that the answer to the problem depends on the behavior of the (n - 2)-nd derivative of the parallel section functions. The affirmative answer to the Busemann-Petty problem for n 4 and the negative answer for n 5 now follow from the fact that convexity controls the second derivatives, but does not control the derivatives of higher orders.

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Annals of Mathematics





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Published by: Annals of Mathematics

Princeton University, Department of Mathematics

Article DOI: 10.2307/120978

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