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相关论文: Critical points of a non-Gaussian random field

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Measures of the non-Gaussianity of a random field depend on how accurately one is able to measure the field. If a signal measured at a certain point is to be averaged with its surroundings, or coarse-grained, the magnitude of its…

统计力学 · 物理学 2015-06-18 T. H. Beuman , A. M. Turner , V. Vitelli

Gaussian random fields pervade all areas of science. However, it is often the departures from Gaussianity that carry the crucial signature of the nonlinear mechanisms at the heart of diverse phenomena, ranging from structure formation in…

统计力学 · 物理学 2015-06-05 T. H. Beuman , A. M. Turner , V. Vitelli

Random fields in nature often have, to a good approximation, Gaussian characteristics. For such fields, the relative densities of umbilical points -- topological defects which can be classified into three types -- have certain fixed values.…

统计力学 · 物理学 2013-08-09 A. M. Turner , T. H. Beuman , V. Vitelli

When the equations that govern the dynamics of a random field are nonlinear, the field can develop with time non-Gaussian statistics even if its initial condition is Gaussian. Here, we provide a general framework for calculating the effect…

统计力学 · 物理学 2013-03-14 T. H. Beuman , A. M. Turner , V. Vitelli

We formulate the statistics of peaks of non-Gaussian random fields and implement it to study the sphericity of peaks. For non-Gaussianity of the local type, we present a general formalism valid regardless of how large the deviation from…

宇宙学与河外天体物理 · 物理学 2025-09-03 Cristiano Germani , Mohammad Ali Gorji , Michiru Uwabo-Niibo , Masahide Yamaguchi

We study the peak height distribution of certain non-stationary Gaussian random fields. The explicit peak height distribution of smooth, non-stationary Gaussian processes in 1D with general covariance is derived. The formula is determined…

统计方法学 · 统计学 2025-02-19 Yu Zhao , Dan Cheng , Samuel Davenport , Armin Schwartzman

In this work we study the properties of the mass density field in the non-Gaussian world models simulated by Grossi et al. 2007. In particular we focus on the one-point density probability distribution function of the mass density field in…

天体物理学 · 物理学 2010-03-26 M. Grossi , E. Branchini , K. Dolag , S. Matarrese , L. Moscardini

Analytic expressions for the statistics of peaks of random fields with weak non-Gaussianity are provided. Specifically, the abundance and spatial correlation of peaks are represented by formulas which can be evaluated only by virtually…

宇宙学与河外天体物理 · 物理学 2020-03-04 Takahiko Matsubara

A flexible model for non-stationary Gaussian random fields on hypersurfaces is introduced.The class of random fields on curves and surfaces is characterized by an amplitude spectral density of a second order elliptic differential…

数值分析 · 数学 2024-12-02 Erik Jansson , Annika Lang , Mike Pereira

We consider fluctuations in the distribution of critical points - saddle points, minima and maxima - of random gaussian fields. We calculate the asymptotic limits of the two point correlation function for various critical point densities,…

无序系统与神经网络 · 物理学 2011-12-12 Avraham Klein , Oded Agam

Critical points of a scalar quantitiy are either extremal points or saddle points. The character of the critical points is determined by the sign distribution of the eigenvalues of the Hessian matrix. For a two-dimensional homogeneous and…

流体动力学 · 物理学 2009-11-13 H. Vogel , W. Mohring

We compute the probability density distribution of maxima for a scalar random field in the presence of local non-gaussianities. The physics outcome of this analysis is the following. If we focus on maxima whose curvature is larger than a…

宇宙学与河外天体物理 · 物理学 2021-09-08 Flavio Riccardi , Marco Taoso , Alfredo Urbano

Motivated by the papers of Mladenovc and Piterbarg (2006), Krajka (2011) and Pereira and Tan (2017), we study the limit properties for the maxima from nonstationary random fields subject to missing observations and obtain the weakly…

概率论 · 数学 2023-06-27 Shengchao Zheng , Zhongquan Tan

The observed abundance of high-redshift galaxies and clusters contains precious information about the properties of the initial perturbations. We present a method to compute analytically the number density of objects as a function of mass…

天体物理学 · 物理学 2011-05-05 Sabino Matarrese , Licia Verde , Raul Jimenez

Using cosmological N-body simulations, we study the abundance of local maxima (peaks) and minima (dips) identified in the smoothed distribution of halos and dark matter (DM) on scales of $10-100$s Mpcs. The simulations include Gaussian and…

宇宙学与河外天体物理 · 物理学 2018-08-08 Adi Nusser , Matteo Biagetti , Vincent Desjacques

We consider the signed density of the extremal points of (two-dimensional) scalar fields with a Gaussian distribution. We assign a positive unit charge to the maxima and minima of the function and a negative one to its saddles. At first, we…

数学物理 · 物理学 2008-11-26 Georg Foltin

We present exact formulas for both the expected number and the height distribution of local maxima (peaks) in two distinct categories of smooth, non-centered Gaussian fields: (i) nonstationary Gaussian processes and (ii) stationary planar…

概率论 · 数学 2024-12-31 Dan Cheng

We investigate the complex Gaussian as well as non-Gaussian distributed random analytical and entire functions (complex entire random field) and calculate their domain of definiteness (radius of convergence) as well as some important…

复变函数 · 数学 2020-11-03 Maria Rosaria Formica , Eugeny Ostrovsky , Leonid Sirota

Gaussian random fields on Euclidean spaces whose variances reach their maximum values at unique points are considered. Exact asymptotic behaviors of probabilities of large absolute maximum of theirs trajectories have been evaluated using…

概率论 · 数学 2019-04-12 Sergey G. Kobelkov , Vladimir I. Piterbarg

Random fields are useful mathematical tools for representing natural phenomena with complex dependence structures in space and/or time. In particular, the Gaussian random field is commonly used due to its attractive properties and…

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