English

A Gaussian kinematic formula

Probability 2007-05-23 v1

Abstract

In this paper we consider probabilistic analogues of some classical integral geometric formulae: Weyl--Steiner tube formulae and the Chern--Federer kinematic fundamental formula. The probabilistic building blocks are smooth, real-valued random fields built up from i.i.d. copies of centered, unit-variance smooth Gaussian fields on a manifold MM. Specifically, we consider random fields of the form fp=F(y1(p),...,yk(p))f_p=F(y_1(p),...,y_k(p)) for FC2(Rk;R)F\in C^2(\mathbb{R}^k;\mathbb{R}) and (y1,...,yk)(y_1,...,y_k) a vector of C2C^2 i.i.d. centered, unit-variance Gaussian fields. The analogue of the Weyl--Steiner formula for such Gaussian-related fields involves a power series expansion for the Gaussian, rather than Lebesgue, volume of tubes: that is, power series expansions related to the marginal distribution of the field ff. The formal expansions of the Gaussian volume of a tube are of independent geometric interest. As in the classical Weyl--Steiner formulae, the coefficients in these expansions show up in a kinematic formula for the expected Euler characteristic, χ\chi, of the excursion sets Mf1[u,+)=My1(F1[u,+))M\cap f^{-1}[u,+\infty)=M\cap y^{-1}(F^{-1}[u,+\infty)) of the field ff. The motivation for studying the expected Euler characteristic comes from the well-known approximation P[suppMf(p)u]E[χ(f1[u,+))]\mathbb{P}[\sup_{p\in M}f(p)\geq u]\simeq\mathbb{E}[\chi(f^{-1}[u,+\infty))].

Keywords

Cite

@article{arxiv.math/0602545,
  title  = {A Gaussian kinematic formula},
  author = {Jonathan E. Taylor},
  journal= {arXiv preprint arXiv:math/0602545},
  year   = {2007}
}

Comments

Published at http://dx.doi.org/10.1214/009117905000000594 in the Annals of Probability (http://www.imstat.org/aop/) by the Institute of Mathematical Statistics (http://www.imstat.org)