Critical points of a non-Gaussian random field
Statistical Mechanics
2012-10-26 v1 Cosmology and Nongalactic Astrophysics
Abstract
Random fields in nature often have, to a good approximation, Gaussian characteristics. We present the mathematical framework for a new and simple method for investigating the non-Gaussian contributions, based on counting the maxima and minima of a scalar field. We consider a random surface, whose height is given by a nonlinear function of a Gaussian field. We find that, as a result of the non-Gaussianity, the density of maxima and minima no longer match and calculate the relative imbalance between the two. Our approach allows to detect and quantify non-Gaussianities present in any random field that can be represented as the height of a smooth two-dimensional surface.
Keywords
Cite
@article{arxiv.1210.6871,
title = {Critical points of a non-Gaussian random field},
author = {T. H. Beuman and A. M. Turner and V. Vitelli},
journal= {arXiv preprint arXiv:1210.6871},
year = {2012}
}
Comments
13 pages, 7 figures