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相关论文: Asymptotic structure of cosmological fluid flows i…

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We study the cosmological Burgers model, as we call it, which is a nonlinear hyperbolic balance law (in one and two spatial variables) posed on an expanding or contracting background. We design a finite volume scheme that is fourth-order in…

偏微分方程分析 · 数学 2019-11-19 Yangyang Cao , Mohammad A. Ghazizadeh , Philippe G. LeFloch

We study the limiting behavior of the solutions of Euler equations of one-dimensional compressible fluid flow as the pressure like term vanishes. This system can be thought of as an approximation for the one dimensional model for large…

偏微分方程分析 · 数学 2018-03-06 Manas Ranjan Sahoo , Abhrojyoti Sen

We consider the gravitational Euler-Poisson system with a linear equation of state on an expanding cosmological model of the Universe. The expansion of the spatial sections introduces an additional dissipating effect in the Euler equation.…

偏微分方程分析 · 数学 2025-12-23 David Fajman , Maciej Maliborski , Maximilian Ofner , Todd Oliynyk , Zoe Wyatt

We present some recent developments on shock capturing methods for nonlinear hyperbolic systems of balance laws, whose prototype is the Euler system of compressible fluid flows, and especially discuss {structure-preserving} techniques. The…

偏微分方程分析 · 数学 2015-12-29 Philippe G. LeFloch

We present a numerical scheme for immiscible two-phase flows with one compressible and one incompressible phase. Special emphasis lies in the discussion of the coupling strategy for compressible and incompressible Euler equations to…

流体动力学 · 物理学 2015-12-11 Jochen Neusser , Veronika Schleper

Considering the isentropic Euler equations of compressible fluid dynamics with geometric effects included, we establish the existence of entropy solutions for a large class of initial data. We cover fluid flows in a nozzle or in spherical…

偏微分方程分析 · 数学 2008-12-16 Philippe G. LeFloch , Michael Westdickenberg

In this paper we introduce a numerical scheme for fluid-structure interaction problems in two or three space dimensions: A flexible elastic plate is interacting with a viscous, compressible barotropic fluid. Hence the physical domain of…

数值分析 · 数学 2020-03-10 Sebastian Schwarzacher , Bangwei She

We study curved isotropic cosmologies filled with two interacting fluids near their time singularities. We find that a number of these universes asymptote to flat limits in the sense that their asymptotic properties become indistinguishable…

广义相对论与量子宇宙学 · 物理学 2013-10-30 Spiros Cotsakis , Georgia Kittou

For the evolution of a compressible fluid in spherical symmetry on a Schwarzschild curved background, we design a class of well-balanced numerical algorithms with first-order or second-order of accuracy. We treat both the relativistic…

数值分析 · 数学 2021-04-27 Philippe G. LeFloch , Carlos Parés , Ernesto Pimentel-García

Self-similar, spherically symmetric cosmological models with a perfect fluid and a scalar field with an exponential potential are investigated. New variables are defined which lead to a compact state space, and dynamical systems methods are…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Alan Coley , Martin Goliath

We consider the relativistic Euler equations governing spherically symmetric, perfect fluid flows on the outer domain of communication of Schwarzschild spacetime, and we introduce a version of the finite volume method which is formulated…

广义相对论与量子宇宙学 · 物理学 2013-01-01 Philippe G. LeFloch , Hasan Makhlof

A recent paper [CGT] studies the evolution of star-shaped mean convex hypersurfaces of the Euclidean space by a class of nonhomogeneous expanding curvature flows. In the present paper we consider the same problem in the real, complex and…

微分几何 · 数学 2020-10-08 Giuseppe Pipoli

Numerical simulation of compressible fluid flows is performed using the Euler equations. They include the scalar advection equation for the density, the vector advection equation for the velocity and a given pressure dependence on the…

计算工程、金融与科学 · 计算机科学 2018-01-22 Petr N. Vabishchevich

We consider a cosmological model in which the two major fluid components of the Universe, dark energy and dark matter, flow with distinct four-velocities. This cosmological configuration is equivalent to a single anisotropic fluid,…

广义相对论与量子宇宙学 · 物理学 2013-07-24 Tiberiu Harko , Francisco S. N. Lobo

We find various asymptotic limits of universes containing two interacting fluids which interact and exchange energy. We study the finite-time singularities that may develop in these cosmologies and obtain the asymptotic behaviours of the…

广义相对论与量子宇宙学 · 物理学 2013-02-20 Spiros Cotsakis , Georgia Kittou

Static spherically symmetric solutions to the Einstein-Euler equations with prescribed central densities are known to exist, be unique and smooth for reasonable equations of state. Some criteria are also available to decide whether…

广义相对论与量子宇宙学 · 物理学 2019-03-01 Lars Andersson , Annegret Y. Burtscher

In this work we study the asymptotic behavior of solutions of the incompressible two-dimensional Euler equations in the exterior of a single smooth obstacle when the obstacle becomes very thin tending to a curve. We extend results by…

偏微分方程分析 · 数学 2015-05-13 Christophe Lacave

We study the asymptotic behavior of solutions of the two dimensional incompressible Euler equations in the exterior of a curve when the curve shrinks to a point. This work links two previous results: [Iftimie, Lopes Filho and Nussenzveig…

偏微分方程分析 · 数学 2011-02-07 Christophe Lacave

We are concerned with underlying connections between fluids, elasticity, isometric embedding of Riemannian manifolds, and the existence of wrinkled solutions of the associated nonlinear partial differential equations. In this paper, we…

偏微分方程分析 · 数学 2017-08-29 Amit Acharya , Gui-Qiang Chen , Siran Li , Marshall Slemrod , Dehua Wang

This paper investigates the asymptotic behavior of the Helmholtz free energy of mixtures at small compressibility. We start from a general representation for the local free energy that is valid in stable subregions of the phase diagram. On…

数学物理 · 物理学 2021-04-20 Dieter Bothe , Wolfgang Dreyer , Pierre-Etienne Druet
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