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We provide a simple formula that accurately approximates the first crossing distribution of barriers having a wide variety of shapes, by random walks with a wide range of correlations between steps. Special cases of it are useful for…

宇宙学与河外天体物理 · 物理学 2013-01-25 Marcello Musso , Ravi K. Sheth

The Excursion Set approach has been used to make predictions for a number of interesting quantities in studies of nonlinear hierarchical clustering. These include the halo mass function, halo merger rates, halo formation times and masses,…

宇宙学与河外天体物理 · 物理学 2012-02-23 Aseem Paranjape , Tsz Yan Lam , Ravi K. Sheth

We describe a simple fully analytic model of the excursion set approach associated with two Gaussian random walks: the first walk represents the initial overdensity around a protohalo, and the second is a crude way of allowing for other…

宇宙学与河外天体物理 · 物理学 2015-06-12 Emanuele Castorina , Ravi K. Sheth

Random walks with a general, nonlinear barrier have found recent applications ranging from reionization topology to refinements in the excursion set theory of halos. Here, we derive the first-crossing distribution of random walks with a…

天体物理学 · 物理学 2009-11-13 Jun Zhang , Lam Hui

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…

宇宙学与河外天体物理 · 物理学 2014-02-18 Arya Farahi , Andrew J. Benson

Insight into a number of interesting questions in cosmology can be obtained from the first crossing distributions of physically motivated barriers by random walks with correlated steps. We write the first crossing distribution as a formal…

宇宙学与河外天体物理 · 物理学 2014-07-09 Marcello Musso , Ravi K. Sheth

We exploit the excursion set approach in integral formulation to derive novel, accurate analytic approximations of the unconditional and conditional first crossing distributions, for random walks with uncorrelated steps and general shapes…

宇宙学与河外天体物理 · 物理学 2015-06-16 A. Lapi , P. Salucci , L. Danese

We study the effects of primordial non-Gaussianity on the large scale structure in the excursion set approach, accounting for correlations between steps of the random walks in the smoothed initial density field. These correlations are…

宇宙学与河外天体物理 · 物理学 2012-02-23 Marcello Musso , Aseem Paranjape

The simplest stochastic halo formation models assume that the traceless part of the shear field acts to increase the initial overdensity (or decrease the underdensity) that a protohalo (or protovoid) must have if it is to form by the…

宇宙学与河外天体物理 · 物理学 2014-07-09 Marcello Musso , Ravi K. Sheth

The excursion set approach uses the statistics of the density field smoothed on a wide range of scales, to gain insight into a number of interesting processes in nonlinear structure formation, such as cluster assembly, merging and…

宇宙学与河外天体物理 · 物理学 2014-10-13 Marcello Musso , Ravi K. Sheth

The excursion set theory, where density perturbations evolve stochastically with the smoothing scale, provides a method for computing the dark matter halo mass function. The computation of the mass function is mapped into the so-called…

宇宙学与河外天体物理 · 物理学 2012-01-05 Andrea De Simone , Michele Maggiore , Antonio Riotto

The excursion set approach provides a framework for predicting how the abundance of dark matter halos depends on the initial conditions. A key ingredient of this formalism comes from the physics of halo formation: the specification of a…

宇宙学与河外天体物理 · 物理学 2014-11-12 I. Achitouv , Y. Rasera , R. K. Sheth , P. S. Corasaniti

We consider a discrete-time random walk on a line starting at $x_0\geq 0$ where a cost is incurred at each jump. We obtain an exact analytical formula for the distribution of the total cost of a trajectory until the process crosses the…

统计力学 · 物理学 2026-02-03 Francesco Mori , Satya N. Majumdar , Pierpaolo Vivo

We describe a model of dark matter halo abundances and clustering which combines the two most widely used approaches to this problem: that based on peaks and the other based on excursion sets. Our approach can be thought of as addressing…

宇宙学与河外天体物理 · 物理学 2015-06-05 Aseem Paranjape , Ravi K. Sheth

If one accounts for correlations between scales, then nonlocal, k-dependent halo bias is part and parcel of the excursion set approach, and hence of halo model predictions for galaxy bias. We present an analysis that distinguishes between a…

宇宙学与河外天体物理 · 物理学 2015-06-05 Marcello Musso , Aseem Paranjape , Ravi K. Sheth

We show how the excursion set moving barrier model for halo abundances may be generalized to the local non-Gaussian f_{nl} model. Our estimate assumes that the distribution of step sizes depends on f_{nl}, but that they are otherwise…

宇宙学与河外天体物理 · 物理学 2015-05-13 Tsz Yan Lam , Ravi K. Sheth

In terms of the excursion set model, we used Monte Carlo methods in order to study the non-Markovian stochastic evolution of the smoothed overdensity $\delta$ at scale $S$. For a Gaussian density field, smoothed by the top-hat filter, in…

宇宙学与河外天体物理 · 物理学 2022-06-23 Nicos Hiotelis

We study first-passage statistics for one-dimensional random walks $S_n$ with independent and identically distributed jumps starting from the origin. We focus on the joint distribution of the first-passage time $\tau_b$ and first-passage…

统计力学 · 物理学 2025-07-16 Mattia Radice , Giampaolo Cristadoro

The excursion set approach allows one to estimate the abundance and spatial distribution of virialized dark matter haloes efficiently and accurately. The predictions of this approach depend on how the nonlinear processes of collapse and…

天体物理学 · 物理学 2009-11-06 Ravi K. Sheth , Giuseppe Tormen

In excursion set theory the computation of the halo mass function is mapped into a first-passage time process in the presence of a barrier, which in the spherical collapse model is a constant and in the ellipsoidal collapse model is a fixed…

宇宙学与河外天体物理 · 物理学 2014-11-18 Michele Maggiore , Antonio Riotto
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