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We present a new approach to computing the matter density power spectrum, from large linear scales to small highly nonlinear scales. Instead of explicitly computing a partial series of high-order diagrams, as in perturbative resummation…

宇宙学与河外天体物理 · 物理学 2013-05-17 Patrick Valageas , Takahiro Nishimichi , Atsushi Taruya

We study the connection of matter density and its tracers from the PDF perspective. One aspect of this connection is the conditional expectation value $\langle \delta_{\mathrm{tracer}}|\delta_m\rangle$ when averaging both tracer and matter…

宇宙学与河外天体物理 · 物理学 2022-01-19 Oliver Friedrich , Anik Halder , Aoife Boyle , Cora Uhlemann , Dylan Britt , Sandrine Codis , Daniel Gruen , ChangHoon Hahn

In modern cosmology, the precision of the theoretical prediction is increasingly required. In cosmological $N$-body simulations, the effect of higher-order Lagrangian perturbation on the initial conditions appears in terms of statistical…

宇宙学与河外天体物理 · 物理学 2021-01-27 Takayuki Tatekawa

Gravitationally collapsed objects are known to be biased tracers of an underlying density contrast. Using symmetry arguments, generalised biasing schemes have recently been developed to relate the halo density contrast $\delta_h$ with the…

宇宙学与河外天体物理 · 物理学 2018-02-14 Dipak Munshi

A consistent guiding-center Hamiltonian theory is derived by Lie-transform perturbation method, with terms up to second order in magnetic-field nonuniformity. Consistency is demonstrated by showing that the guiding-center transformation…

等离子体物理 · 物理学 2015-12-09 Natalia Tronko , Alain Brizard

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

We derive, using functional methods and the bias expansion, the conditional likelihood for observing a specific tracer field given an underlying matter field. This likelihood is necessary for Bayesian-inference methods. If we neglect all…

宇宙学与河外天体物理 · 物理学 2020-05-06 Giovanni Cabass , Fabian Schmidt

We investigate the building of unified models that can predict the matter-density power spectrum and the two-point correlation function from very large to small scales, being consistent with perturbation theory at low $k$ and with halo…

宇宙学与河外天体物理 · 物理学 2015-05-19 Patrick Valageas , Takahiro Nishimichi

We develop a simple formalism of biased tracers that we dub $\mathit{Monkey\ bias}$. In this formalism, a biased tracer field is constructed directly in terms of the linear matter fluctuation field and the set of derivative operators acting…

宇宙学与河外天体物理 · 物理学 2020-11-20 Tomohiro Fujita , Zvonimir Vlah

The relativistic generalization of the Newtonian Lagrangian perturbation theory is investigated. In previous works, the perturbation and solution schemes that are generated by the spatially projected gravitoelectric part of the Weyl tensor…

广义相对论与量子宇宙学 · 物理学 2018-01-01 Fosca Al Roumi , Thomas Buchert , Alexander Wiegand

With the completion of the Planck mission, in order to continue to gather cosmological information it has become crucial to understand the Large Scale Structures (LSS) of the universe to percent accuracy. The Effective Field Theory of LSS…

宇宙学与河外天体物理 · 物理学 2016-02-23 Raul Angulo , Matteo Fasiello , Leonardo Senatore , Zvonimir Vlah

In this work, the benefits of the phase fitting technique are embedded in high order discrete Lagrangian integrators. The proposed methodology creates integrators with zero phase lag in a test Lagrangian in a similar way used in phase…

天体物理仪器与方法 · 物理学 2009-04-02 O. T. Kosmas , D. S. Vlachos

We make use of neural networks to accelerate the calculation of power spectra required for the analysis of galaxy clustering and weak gravitational lensing data. For modern perturbation theory codes, evaluation time for a single cosmology…

宇宙学与河外天体物理 · 物理学 2022-05-11 Joseph DeRose , Shi-Fan Chen , Martin White , Nickolas Kokron

We investigate sources of error in acceleration statistics from Lagrangian Particle Tracking (LPT) data and demonstrate techniques to eliminate or minimise bias errors introduced during processing. Numerical simulations of particle tracking…

流体动力学 · 物理学 2018-11-14 John M. Lawson , Eberhard Bodenschatz , Cristian C. Lalescu , Michael Wilczek

We test tree-level perturbation theory for Gaussian initial conditions with power spectra $P(k)\propto k^n$ by comparing the probability distribution function (PDF) for the density predicted by the Local Lagrangian Approximation (LLA) with…

天体物理学 · 物理学 2015-06-24 Zacharias A. M. Protogeros , Adrian L. Melott , Robert J. Scherrer

The nonlinear perturbation theory of gravitational instability is extended to include effects of both biasing and redshift-space distortions, which are inevitable in predicting observable quantities in galaxy surveys. The precise…

天体物理学 · 物理学 2014-11-18 Takahiko Matsubara

Analyzing the clustering of galaxies at the field level in principle promises access to all the cosmological information available. Given this incentive, in this paper we investigate the performance of field-based forward modeling approach…

宇宙学与河外天体物理 · 物理学 2023-07-31 Andrija Kostić , Nhat-Minh Nguyen , Fabian Schmidt , Martin Reinecke

We demonstrate the effectiveness of one of the many multi-tracer analyses enabled by Optimal Transport (OT) reconstruction. Leveraging a semi-discrete OT algorithm, we determine the displacements between initial and observed positions of…

宇宙学与河外天体物理 · 物理学 2024-03-19 Farnik Nikakhtar , Ravi K. Sheth , Nikhil Padmanabhan , Bruno Lévy , Roya Mohayaee

We review a perturbative approach to deal with Lagrangians with higher or infinite order time derivatives. It enables us to construct a consistent Poisson structure and Hamiltonian with only first time derivatives order by order in…

高能物理 - 理论 · 物理学 2008-11-26 Tai-Chung Cheng , Pei-Ming Ho , Mao-Chuang Yeh

There is a growing attention given to utilizing Lagrangian and Hamiltonian mechanics with network training in order to incorporate physics into the network. Most commonly, conservative systems are modeled, in which there are no frictional…

机器学习 · 计算机科学 2024-05-28 Veera Sundararaghavan , Megna N. Shah , Jeff P. Simmons