A relaxation scheme for inviscid flows under gravitational influence

Many astrophysical flows are modeled by the Euler equations with gravity source terms derived from a potential, the evolution of which is described by a Poisson equation. Several gravitational flows reach equilibrium states that are necessary to preserve in the numerica...

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Main Authors: Vides Jeaniffer, Audit Edouard, Nkonga Boniface
Format: Article
Language:English
Published: EDP Sciences 2014-09-01
Series:ESAIM: Proceedings and Surveys
Online Access:http://dx.doi.org/10.1051/proc/201445054
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author Vides Jeaniffer
Audit Edouard
Nkonga Boniface
author_facet Vides Jeaniffer
Audit Edouard
Nkonga Boniface
author_sort Vides Jeaniffer
collection DOAJ
description Many astrophysical flows are modeled by the Euler equations with gravity source terms derived from a potential, the evolution of which is described by a Poisson equation. Several gravitational flows reach equilibrium states that are necessary to preserve in the numerical formulation. In this paper, we present the derivation of the relaxation model ? , in which the pressure is a supplementary variable and the Poisson equation is transformed into a hyperbolic equation with a penalty parameter. The corresponding scheme is obtained in the limit as the parameter tends to zero. The proposed Riemann solver, implemented in the software HERACLES ? , provides better robustness compared to other approaches available in the same software and is capable of preserving gravitational equilibria when required. Several numerical tests and results are presented, as well.
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spelling doaj.art-753744e4b53a4272a195c7ed465f37812023-01-03T03:32:04ZengEDP SciencesESAIM: Proceedings and Surveys2267-30592014-09-014552353210.1051/proc/201445054proc144554A relaxation scheme for inviscid flows under gravitational influenceVides Jeaniffer0Audit Edouard1Nkonga Boniface2Inria, Maison de la SimulationCEA, Maison de la SimulationUniversité de Nice-Sophia AntipolisMany astrophysical flows are modeled by the Euler equations with gravity source terms derived from a potential, the evolution of which is described by a Poisson equation. Several gravitational flows reach equilibrium states that are necessary to preserve in the numerical formulation. In this paper, we present the derivation of the relaxation model ? , in which the pressure is a supplementary variable and the Poisson equation is transformed into a hyperbolic equation with a penalty parameter. The corresponding scheme is obtained in the limit as the parameter tends to zero. The proposed Riemann solver, implemented in the software HERACLES ? , provides better robustness compared to other approaches available in the same software and is capable of preserving gravitational equilibria when required. Several numerical tests and results are presented, as well.http://dx.doi.org/10.1051/proc/201445054
spellingShingle Vides Jeaniffer
Audit Edouard
Nkonga Boniface
A relaxation scheme for inviscid flows under gravitational influence
ESAIM: Proceedings and Surveys
title A relaxation scheme for inviscid flows under gravitational influence
title_full A relaxation scheme for inviscid flows under gravitational influence
title_fullStr A relaxation scheme for inviscid flows under gravitational influence
title_full_unstemmed A relaxation scheme for inviscid flows under gravitational influence
title_short A relaxation scheme for inviscid flows under gravitational influence
title_sort relaxation scheme for inviscid flows under gravitational influence
url http://dx.doi.org/10.1051/proc/201445054
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