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We present a new method to calculate formation of cosmological structure in the Newtonian limit. The method is based on Lagrangian perturbation theory plus two key theoretical extensions. One advance involves identifying and fixing a…

宇宙学与河外天体物理 · 物理学 2014-12-15 Sharvari Nadkarni-Ghosh , David F. Chernoff

We explore the Lagrangian perturbation theory (LPT) at 1-loop order with Gaussian initial conditions. We present an expansion method to approximately compute the power spectrum in LPT. Our approximate solution has good convergence in the…

宇宙学与河外天体物理 · 物理学 2015-06-17 Naonori S. Sugiyama

We present a simple and intuitive approximation for solving perturbation theory (PT) of small cosmic fluctuations. We consider only the spherically symmetric or monopole contribution to the PT integrals, which yields the exact result for…

天体物理学 · 物理学 2009-10-30 P. Fosalba , E. Gaztanaga

We study Lagrangian Perturbation Theory (LPT) and its regularization in the Effective Field Theory (EFT) approach. We evaluate the LPT displacement with the same phases as a corresponding $N$-body simulation, which allows us to compare…

宇宙学与河外天体物理 · 物理学 2016-03-23 Tobias Baldauf , Emmanuel Schaan , Matias Zaldarriaga

Many models of high energy physics suggest that the cosmological dark sector consists of not just one, but a spectrum of ultralight scalar particles with logarithmically distributed masses. To study the potential signatures of low…

宇宙学与河外天体物理 · 物理学 2021-03-17 Alex Laguë , J. Richard Bond , Renée Hložek , David J. E. Marsh , Laurin Söding

This is part two in a series of papers in which we investigate an approach based on Lagrangian perturbation theory (LPT) to study the non-linear evolution of the large-scale structure distribution in the universe. Firstly, we compute the…

宇宙学与河外天体物理 · 物理学 2012-06-15 Cornelius Rampf , Yvonne Y. Y. Wong

In the standard perturbation theory (SPT) of self-gravitating Newtonian fluid in an expanding universe, recurrence relations for higher-order solutions are well known and play an important role both in practical applications and in…

宇宙学与河外天体物理 · 物理学 2015-08-12 Takahiko Matsubara

Galaxy surveys demand fast large-scale structure forward models that preserve large-scale phases while providing realistic nonlinear morphology at fixed force resolution. Single-step Lagrangian Perturbation Theory (LPT) solvers are…

宇宙学与河外天体物理 · 物理学 2026-03-26 Francisco-Shu Kitaura , Francesco Sinigaglia

We derive a recursion relation in the framework of Lagrangian perturbation theory, appropriate for studying the inhomogeneities of the large scale structure of the universe. We use the fact that the perturbative expansion of the matter…

宇宙学与河外天体物理 · 物理学 2014-03-27 Cornelius Rampf

A common ingredient in cosmological perturbation theory (PT) is the expansion of the dark matter overdensity $\delta$ in the Lagrangian displacement $s$, which amounts to enforcing mass conservation perturbatively. In Eulerian PT (EPT),…

宇宙学与河外天体物理 · 物理学 2026-05-29 Svetlin V. Tassev

We present a new fast and efficient approach to model structure formation with Augmented Lagrangian Perturbation Theory (ALPT). Our method is based on splitting the displacement field into a long and a short-range component. The long-range…

宇宙学与河外天体物理 · 物理学 2015-06-12 Francisco-Shu Kitaura , Steffen Heß

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

We develop a Lagrangian Perturbation Theory (LPT) framework to study the clustering of cold dark matter (CDM) in cosmologies with massive neutrinos. We follow the trajectories of CDM particles with Lagrangian displacements fields up to…

宇宙学与河外天体物理 · 物理学 2020-10-28 Alejandro Aviles , Arka Banerjee

Context: Analyzing the large-scale structure (LSS) with galaxy surveys demands accurate structure formation models. Such models should ideally be fast and have a clear theoretical framework to rapidly scan a variety of cosmological…

宇宙学与河外天体物理 · 物理学 2024-02-08 F. -S. Kitaura , F. Sinigaglia , A. Balaguera-Antolínez , G. Favole

A general theoretical framework that incorporates possible CPT and Lorentz violation in an extension of the standard model and in quantum electrodynamics has been developed over the last decade. The framework originates in the idea that CPT…

高能物理 - 唯象学 · 物理学 2007-05-23 Neil Russell

We present \emph{Unified Lagrangian Perturbation Theory} (ULPT), a perturbative framework for consistently modeling galaxy density fluctuations across real space, redshift space, and post-reconstruction fields. Unlike existing approaches…

宇宙学与河外天体物理 · 物理学 2025-09-08 Naonori Sugiyama

Motivated by robotic trajectory optimization problems we consider the Augmented Lagrangian approach to constrained optimization. We first propose an alternative augmentation of the Lagrangian to handle the inequality case (not based on…

最优化与控制 · 数学 2014-12-16 Marc Toussaint

We explore the relationship between the nonlinear matter power spectrum and the various Lagrangian and Standard Perturbation Theories (LPT and SPT). We first look at it in the context of one dimensional (1-d) dynamics, where 1LPT is exact…

宇宙学与河外天体物理 · 物理学 2016-05-03 Zvonimir Vlah , Uroš Seljak , Man Yat Chu , Yu Feng

Perturbation theory is an indispensable tool for studying the cosmic large-scale structure, and establishing its limits is therefore of utmost importance. One crucial limitation of perturbation theory is shell-crossing, which is the…

宇宙学与河外天体物理 · 物理学 2021-06-25 Cornelius Rampf , Oliver Hahn

On the smallest scales, three-dimensional large-scale structure surveys contain a wealth of cosmological information which cannot be trivially extracted due to the non-linear dynamical evolution of the density field. Lagrangian perturbation…

宇宙学与河外天体物理 · 物理学 2015-08-05 Florent Leclercq , Jens Jasche , Héctor Gil-Marín , Benjamin Wandelt
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