English

Statistics of Peaks in Chi-Squared Fields

Mathematical Physics 2018-10-05 v1 Cosmology and Nongalactic Astrophysics math.MP

Abstract

Chi-squared random fields arise naturally from the study of fluctuations in field theories with SO(n) symmetry. The extrema of chi-squared fields are of particular physical interest. In this paper, we undertake a statistical analysis of the stationary points of chi-squared fields, with particular emphasis on extrema. We begin by describing the neighborhood of a stationary point in terms of a biased chi-squared random field, and then compute the expected profile of this field, as well as a variety of associated statistics. We are interested in understanding how spherically symmetric the neighborhood of a stationary point is, on average. To this end, we decompose the biased field into its spherical harmonic modes about this point, and explore their statistics. Using these mode statistics, we construct a metric to gauge the degree of spherical symmetry of the field in this neighborhood. Finally, we show how to leverage the harmonic decomposition to efficiently sample both Gaussian and chi-squared fields about a stationary point.

Keywords

Cite

@article{arxiv.1810.02078,
  title  = {Statistics of Peaks in Chi-Squared Fields},
  author = {Jolyon K. Bloomfield and Stephen H. P. Face and Alan H. Guth and Saarik Kalia and Zander Moss},
  journal= {arXiv preprint arXiv:1810.02078},
  year   = {2018}
}

Comments

38 pages + 11 pages of appendices, 5 figures

R2 v1 2026-06-23T04:28:08.139Z