English

Excursion Set Theory for Correlated Random Walks

Cosmology and Nongalactic Astrophysics 2014-02-18 v2

Abstract

We present a new method to compute the first crossing distribution in excursion set theory for the case of correlated random walks. We use a combination of the path integral formalism of Maggiore & Riotto, and the integral equation solution of Zhang & Hui, and Benson et al. to find a numerically robust and convenient algorithm to derive the first crossing distribution in terms of a perturbative expansion around the limit of an uncorrelated random walk. We apply this methodology to the specific case of a Gaussian random density field filtered with a Gaussian smoothing function. By comparing our solutions to results from Monte Carlo calculations of the first crossing distribution we demonstrate that our method accurate for power spectra P(k)knP(k)\propto k^n for n=1n=1, becoming less accurate for smaller values of nn. It is therefore complementary to the method of Musso & Sheth, which will therefore be more useful for standard Λ\LambdaCDM power spectra. Our approach is quite general, and can be adapted to other smoothing functions, and also to non-Gaussian density fields.

Keywords

Cite

@article{arxiv.1303.0337,
  title  = {Excursion Set Theory for Correlated Random Walks},
  author = {Arya Farahi and Andrew J. Benson},
  journal= {arXiv preprint arXiv:1303.0337},
  year   = {2014}
}

Comments

15 pages, 7 figures, Accepted for publication in MNRAS. Some corrections following comments from referee

R2 v1 2026-06-21T23:35:21.825Z