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The Lagrangian perturbation theory provides a simple yet powerful way of computing the nonlinear matter power spectrum, and it has been applied to biased tracers such as halos and galaxies. The number conservation of matter particles allows…

宇宙学与河外天体物理 · 物理学 2025-04-08 Peter Espenshade , Jaiyul Yoo

A forward model of matter and biased tracers at arbitrary order in Lagrangian perturbation theory (LPT) is presented. The forward model contains the complete LPT displacement field at any given order in perturbations, as well as all…

宇宙学与河外天体物理 · 物理学 2021-10-04 Fabian Schmidt

It has been recognized that the observables of large-scale structure (LSS) is susceptible to long-wavelength density and tidal fluctuations whose wavelengths exceed the accessible scale of a finite-volume observation, referred to as the…

宇宙学与河外天体物理 · 物理学 2021-12-02 Atsushi Taruya , Kazuyuki Akitsu

We investigate the statistical properties of Lagrangian tracers transported by a time-correlated compressible renewing flow. We show that the preferential sampling of the phase space performed by tracers yields significant differences…

流体动力学 · 物理学 2015-06-23 Ajinkya Dhanagare , Stefano Musacchio , Dario Vincenzi

The Lagrangian statistics of heavy particles and of fluid tracers transported by a fully developed turbulent flow are investigated by means of high resolution direct numerical simulations. The Lagrangian velocity structure functions are…

混沌动力学 · 物理学 2007-05-23 Jeremie Bec , Luca Biferale , Massimo Cencini , Alessandra S. Lanotte , Federico Toschi

The relationship between observed tracers such as galaxies and the underlying dark matter distribution is crucial in extracting cosmological information. As the linear bias model breaks down at quasi-linear scales, the standard perturbative…

宇宙学与河外天体物理 · 物理学 2015-06-04 Xin Wang , Alex Szalay

We study the effect of turbulence on a sedimenting layer of particles by means of direct numerical simulations. A Lagrangian model in which particles are considered as tracers with an additional downward settling velocity is integrated…

流体动力学 · 物理学 2020-07-08 Alessandro Sozza , Gabor Drotos , Emilio Hernández-García , Cristóbal López

We study the effect of time evolution on galaxy bias. We argue that at any order in perturbations, the galaxy density contrast can be expressed in terms of a finite set of locally measurable operators made of spatial and temporal…

宇宙学与河外天体物理 · 物理学 2015-08-06 Mehrdad Mirbabayi , Fabian Schmidt , Matias Zaldarriaga

Halos are biased tracers of the dark matter distribution. It is often assumed that the patches from which halos formed are locally biased with respect to the initial fluctuation field, meaning that the halo-patch fluctuation field can be…

宇宙学与河外天体物理 · 物理学 2013-04-08 Ravi K. Sheth , Kwan Chuen Chan , Roman Scoccimarro

We investigate the nonlocal behavior of passive tracer dispersion with random stopping at various sites in fluids. This kind of dispersion processes is modeled by an integral partial differential equation, i.e., an advection-diffusion…

动力系统 · 数学 2025-10-20 Jinqiao Duan , James R. Brannan , H. Gao

Non-linear latent variable models have become increasingly popular in a variety of applications. However, there has been little study on theoretical properties of these models. In this article, we study rates of posterior contraction in…

统计理论 · 数学 2011-09-26 Debdeep Pati , Anirban Bhattacharya , David B. Dunson

We discuss the effects of non-linear structure formation on the signature of acoustic oscillations in the late-time galaxy distribution. We argue that the dominant non-linear effect is the differential motion of pairs of tracers separated…

天体物理学 · 物理学 2009-08-18 Daniel J. Eisenstein , Hee-jong Seo , Martin White

Non-linear latent variable models have become increasingly popular in a variety of applications. However, there has been little study on theoretical properties of these models. In this article, we study rates of posterior contraction in…

统计理论 · 数学 2017-01-27 Shuang Zhou , Debdeep Pati , Anirban Bhattacharya , David Dunson

We study aggregation driven by a localized source of monomers. The densities become stationary and have algebraic tails far away from the source. We show that in a model with mass-independent reaction rates and diffusion coefficients, the…

统计力学 · 物理学 2015-06-09 P. L. Krapivsky

In this study, we start from a Follow-the-Leaders model for traffic flow that is based on a weighted harmonic mean (in Lagrangian coordinates) of the downstream car density. This results in a nonlocal Lagrangian partial differential…

偏微分方程分析 · 数学 2024-01-09 Giuseppe M. Coclite , Kenneth H. Karlsen , Nils Henrik Risebro

The dark matter halos that host galaxies and clusters form out of initial high-density patches, providing a biased tracer of the linear matter density field. In the simplest local bias approximation, the halo field is treated as a…

宇宙学与河外天体物理 · 物理学 2016-04-15 Titouan Lazeyras , Marcello Musso , Vincent Desjacques

Recent development in the reconstruction of the large-scale structure (LSS) has seen significant improvement in restoring the linear baryonic acoustic oscillation (BAO) from at least the non-linear matter field. This outstanding performance…

宇宙学与河外天体物理 · 物理学 2019-01-23 Xin Wang , Ue-Li Pen

We study analytically the dynamics and the micro-structural changes of a host medium caused by a driven tracer particle moving in a confined, quiescent molecular crowding environment. Imitating typical settings of active micro-rheology…

统计力学 · 物理学 2016-03-17 O. Bénichou , P. Illien , G. Oshanin , A. Sarracino , R. Voituriez

Lagrangian data assimilation exploits the trajectories of moving tracers as observations to recover the underlying flow field. One major challenge in Lagrangian data assimilation is the intrinsic nonlinearity that impedes using exact…

动力系统 · 数学 2023-06-14 Nan Chen , Shubin Fu

Local-type primordial non-Gaussianity (PNG), predicted by many non-minimal models of inflation, creates a scale-dependent contribution to the power spectrum of large-scale structure (LSS) tracers. Its amplitude is characterized by the…

宇宙学与河外天体物理 · 物理学 2025-02-03 Boryana Hadzhiyska , Simone Ferraro
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