English

Inverse formula for the Blaschke-Levy representation with applications to zonoids and sections of star bodies

Functional Analysis 2016-09-06 v1 Metric Geometry

Abstract

We say that an even continuous function HH on the unit sphere Ω\Omega in RnR^n admits the Blaschke-Levy representation with q>0q>0 if there exists an even function bL1(Ω)b\in L_1(\Omega) so that Hq(x)=Ω(x,ξ)qb(ξ) dξH^q(x)=\int_\Omega |(x,\xi)|^q b(\xi)\ d\xi for every xΩ.x\in \Omega. This representation has numerous applications in convex geometry, probability and Banach space theory. In this paper, we present a simple formula (in terms of the derivatives of HH) for calculating bb out of H.H. We use this formula to give a sufficient condition for isometric embedding of a space into LpL_p which contributes to the 1937 P.Levy's problem and to the study of zonoids. Another application gives a Fourier transform formula for the volume of (n1)(n-1)-dimensional central sections of star bodies in Rn.R^n. We apply this formula to find the minimal and maximal volume of central sections of the unit balls of the spaces pn\ell_p^n with 0<p<2.0<p<2.

Keywords

Cite

@article{arxiv.math/9605212,
  title  = {Inverse formula for the Blaschke-Levy representation with applications to zonoids and sections of star bodies},
  author = {Alexander Koldobsky},
  journal= {arXiv preprint arXiv:math/9605212},
  year   = {2016}
}