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相关论文: Behaviour of Lagrangian Approximations in Spherica…

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We report the findings of new exact analytical solutions to the cosmological fluid equations, namely for the case where the initial conditions are perturbatively close to a spherical top-hat profile. To do so we enable a fluid description…

宇宙学与河外天体物理 · 物理学 2019-02-28 Cornelius Rampf

The wave function in the quantum theory of the O(N) extended supersymmetric particle model describes a massless free field with spin N/2. This quantum theory is here exactly solved in terms of gauge fields in arbitrary even dimensions using…

高能物理 - 理论 · 物理学 2009-06-12 Robert Marnelius

We analyzed the performance of a perturbation theory for nonlinear cosmological dynamics, based on the Lagrangian description of hydrodynamics. In our previous paper, we solved hydrodynamic equations for a self-gravitating fluid with…

天体物理学 · 物理学 2009-11-10 Takayuki Tatekawa

We consider the growth of primordial dark matter halos seeded by three crossed initial sine waves of various amplitudes. Using a Lagrangian treatment of cosmological gravitational dynamics, we examine the convergence properties of a…

宇宙学与河外天体物理 · 物理学 2018-12-18 Shohei Saga , Atsushi Taruya , Stéphane Colombi

Lagrangian perturbation theory for cosmological fluid describes structure formation in the quasi-nonlinear stage well. We present a third-order perturbative equation for Lagrangian perturbation with pressure in both the longitudinal and…

天体物理学 · 物理学 2009-11-10 Takayuki Tatekawa

We describe and test a new method for creating initial conditions for cosmological N-body dark matter simulations based on second-order Lagrangian perturbation theory (2lpt). The method can be applied to multi-mass particle distributions…

宇宙学与河外天体物理 · 物理学 2015-05-14 Adrian Jenkins

We investigate convergence of Lagrangian Perturbation Theory (LPT) by analyzing the model problem of a spherical homogeneous top-hat in an Einstein-deSitter background cosmology. We derive the formal structure of the LPT series expansion,…

宇宙学与河外天体物理 · 物理学 2012-11-27 Sharvari Nadkarni-Ghosh , David F. Chernoff

We investigate the performance of Lagrangian perturbation theory up to the second order for two scenarios of cosmological large-scale structure formation, SCDM (standard cold dark matter) and BSI (broken scale invariance). The latter model…

天体物理学 · 物理学 2015-06-24 Arno G. Weiss , Stefan Gottloeber , Thomas Buchert

We report on the performance of Lagrangian perturbation theory up to the second order for the standard cold dark matter (SCDM) and broken scale invariance (BSI) scenarios. We normalize both models to the COBE data, the BSI model serves as…

天体物理学 · 物理学 2007-05-23 A. G. Weiss , S. Gottloeber , T. Buchert

We study the Lagrangian dynamics of systems of N point vortices and passive particles in a two-dimensional, doubly periodic domain. The probability distribution function of vortex velocity, p_N, has a slow-velocity Gaussian component and a…

chao-dyn · 物理学 2009-10-31 Jeffrey B. Weiss , Antonello Provenzale , James C. McWilliams

We investigate the Lagrangian perturbation theory of a homogeneous and isotropic universe in the non-relativistic limit, and derive the solutions up to the fourth order. These solutions are needed for example for the next-to-leading order…

宇宙学与河外天体物理 · 物理学 2012-06-15 Cornelius Rampf , Thomas Buchert

We present a perturbative treatment of the evolution under their mutual self-gravity of particles displaced off an infinite perfect lattice, both for a static space and for a homogeneously expanding space as in cosmological N-body…

天体物理学 · 物理学 2009-11-11 B. Marcos , T. Baertschiger , M. Joyce , A. Gabrielli , F. Sylos Labini

These lectures notes give an introduction to the fast developing area of research dealing with perturbative descriptions of the gravitational instability in an expanding universe. I just sketch the outlines of some proofs, and many…

天体物理学 · 物理学 2007-05-23 F. R. Bouchet

We study static symmetric solutions in the context of a gravitational theory based on a action-dependent Lagrangian. Such theory has been designed as a setup to implement dissipative effects into the traditional principle of least action.…

广义相对论与量子宇宙学 · 物理学 2019-06-26 Julio C. Fabris , Hermano Velten , Aneta Wojnar

In cubic-order Horndeski theories where a scalar field $\phi$ is coupled to nonrelativistic matter with a field-dependent coupling $Q(\phi)$, we derive the most general Lagrangian having scaling solutions on the isotropic and homogenous…

广义相对论与量子宇宙学 · 物理学 2018-12-27 Noemi Frusciante , Ryotaro Kase , Nelson J. Nunes , Shinji Tsujikawa

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

Sphere packings in high dimensions interest mathematicians and physicists and have direct applications in communications theory. Remarkably, no one has been able to provide exponential improvement on a 100-year-old lower bound on the…

度量几何 · 数学 2007-05-23 S. Torquato , F. H. Stillinger

We examine Lagrangian techniques for computing underapproximations of finite-time horizon, stochastic reach-avoid level-sets for discrete-time, nonlinear systems. We use the concept of reachability of a target tube in the control literature…

系统与控制 · 计算机科学 2017-04-13 Joseph D. Gleason , Abraham P. Vinod , Meeko. M. K. Oishi

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

Using a diagrammatic approach to Eulerian perturbation theory, we analytically calculate the variance and skewness of the density and velocity divergence induced by gravitational evolution from Gaussian initial conditions, including…

天体物理学 · 物理学 2011-09-30 Roman Scoccimarro , Joshua Frieman