Search results for "Riemann solver"

showing 10 items of 22 documents

Adaptive discontinuous evolution Galerkin method for dry atmospheric flow

2014

We present a new adaptive genuinely multidimensional method within the framework of the discontinuous Galerkin method. The discontinuous evolution Galerkin (DEG) method couples a discontinuous Galerkin formulation with approximate evolution operators. The latter are constructed using the bicharacteristics of multidimensional hyperbolic systems, such that all of the infinitely many directions of wave propagation are considered explicitly. In order to take into account multiscale phenomena that typically appear in atmospheric flows nonlinear fluxes are split into a linear part governing the acoustic and gravitational waves and a nonlinear part that models advection. Time integration is realiz…

Backward differentiation formulasteady statesPhysics and Astronomy (miscellaneous)Wave propagationdry atmospheric convectionlarge time stepsystems of hyperbolic balance lawssymbols.namesakeDiscontinuous Galerkin methodApplied mathematicsevolution Galerkin schemesGalerkin methodMathematicssemi-implicit approximationNumerical AnalysisAdaptive mesh refinementApplied MathematicsEuler equationsRiemann solverComputer Science ApplicationsEuler equationsComputational MathematicsNonlinear systemClassical mechanicsModeling and SimulationsymbolsJournal of Computational Physics
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General Relativistic Hydrodynamics and Magnetohydrodynamics: Hyperbolic Systems in Relativistic Astrophysics

2008

Black holePhysicssymbols.namesakeNeutron starRiemann problemActive galactic nucleusClassical mechanicssymbolsRelativistic astrophysicsMagnetohydrodynamicsCenter of mass (relativistic)Riemann solverMathematical physics
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Stellar hydrodynamics with glaister's riemann solver: An approach to the stellar collapse

1990

La resolution de Remann approximee de la solution des equations d'Euler de la dynamique des gaz 1 D, developpee par Glaister P. (1988, J. Comput. Phys., 74) est introduite dans un code hydrodynamique lagrangien et appliquee a l'effondrement stellaire a symetrie spherique

Cauchy problemPhysicsNumerical AnalysisPhysics and Astronomy (miscellaneous)Applied MathematicsWhite dwarfGas dynamicsRiemann solverComputer Science ApplicationsComputational MathematicsSupernovasymbols.namesakeClassical mechanicsModeling and SimulationGravitational collapsesymbolsCircular symmetryStellar evolutionJournal of Computational Physics
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Approximate Osher–Solomon schemes for hyperbolic systems

2016

This paper is concerned with a new kind of Riemann solvers for hyperbolic systems, which can be applied both in the conservative and nonconservative cases. In particular, the proposed schemes constitute a simple version of the classical Osher-Solomon Riemann solver, and extend in some sense the schemes proposed in Dumbser and Toro (2011) 19,20. The viscosity matrix of the numerical flux is constructed as a linear combination of functional evaluations of the Jacobian of the flux at several quadrature points. Some families of functions have been proposed to this end: Chebyshev polynomials and rational-type functions. Our schemes have been tested with different initial value Riemann problems f…

Chebyshev polynomialsApplied MathematicsNumerical analysisMathematical analysis010103 numerical & computational mathematics01 natural sciencesRiemann solverEuler equations010101 applied mathematicsComputational Mathematicssymbols.namesakeRiemann hypothesisRiemann problemJacobian matrix and determinantsymbols0101 mathematicsShallow water equationsMathematicsApplied Mathematics and Computation
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Fine-Mesh Numerical Simulations for 2D Riemann Problems with a Multilevel Scheme

2001

The numerical simulation of physical problems modeled by systems of conservation laws can be difficult due to the occurrence of discontinuities and other non-smooth features in the solution.

Conservation lawComputer simulationAdaptive mesh refinementGodunov's schemeClassification of discontinuitiesTopologyRiemann solversymbols.namesakeRiemann problemMesh generationsymbolsApplied mathematicsComputer Science::DatabasesMathematics
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Riemann solvers in relativistic astrophysics

1999

AbstractOur contribution reviews High Resolution Shock Capturing methods (HRSC) in the field of relativistic hydrodynamics with special emphasis on Riemann solvers. HRSC techniques achieve highly accurate numerical approximations (formally second order or better) in smooth regions of the flow, and capture the motion of unresolved steep gradients without creating spurious oscillations. One objective of our contribution is to show how these techniques have been extended to relativistic hydrodynamics, making it possible to explore some challenging astrophysical scenarios. We will review recent literature concerning the main properties of different special relativistic Riemann solvers, and disc…

Conservation lawPartial differential equationApplied MathematicsRiemann solverLorentz factorsymbols.namesakeTheoretical physicsRiemann hypothesisComputational MathematicsRiemann problemFlow (mathematics)Shock capturing methodsymbolsMathematicsMathematical physicsJournal of Computational and Applied Mathematics
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An HLLC Riemann solver for resistive relativistic magnetohydrodynamics

2017

We present a new approximate Riemann solver for the augmented system of equations of resistive relativistic magnetohydrodynamics (RRMHD) that belongs to the family of Harten-Lax-van Leer contact wave (HLLC) solvers. In HLLC solvers, the solution is approximated by two constant states flanked by two shocks separated by a contact wave. The accuracy of the new approximate solver is calibrated through one- and two-dimensional test problems.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsShock waveResistive touchscreenFOS: Physical sciencesAstronomy and AstrophysicsSolverSystem of linear equations01 natural sciencesRiemann solver010305 fluids & plasmassymbols.namesakeClassical mechanicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesComputer Science::Mathematical SoftwaresymbolsMagnetohydrodynamicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaConstant (mathematics)Instrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Monthly Notices of the Royal Astronomical Society
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High-order methods for the simulation of hydromagnetic instabilities in core-collapse supernovae

2011

AbstractWe present an assessment of the accuracy of a recently developed MHD code used to study hydromagnetic flows in supernovae and related events. The code, based on the constrained transport formulation, incorporates unprecedented ultra-high-order methods (up to 9th order) for the reconstruction and the most accurate approximate Riemann solvers. We estimate the numerical resistivity of these schemes in tearing instability simulations.

PhysicsAstronomy and Astrophysics010103 numerical & computational mathematics01 natural sciencesInstabilityRiemann solverNumerical resistivity010305 fluids & plasmasComputational physicsRoe solverSupernovasymbols.namesakeRiemann problemSpace and Planetary Science0103 physical sciencesTearingsymbols0101 mathematicsMagnetohydrodynamicsProceedings of the International Astronomical Union
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Numerical Relativistic Hydrodynamics

2008

High Resolution Shock Capturing (HRSC) techniques achieve highly accurate numerical approximations (formally second order or better) in smooth regions of the flow, and capture the motion of unresolved steep gradients without creating spurious oscillations. I will show how these techniques have been extended to relativistic hydrodynamics, making it possible to explore some challenging astrophysical scenarios. I will review recent literature concerning the main properties of different special relativistic Riemann solvers, and discuss several test problems which are commonly used to evaluate the performance of numerical methods in relativistic hydrodynamics. In the second part, I will illustra…

PhysicsBlack holeLorentz factorsymbols.namesakeClassical mechanicsRiemann problemActive galactic nucleusAccretion (meteorology)Flow (mathematics)Astrophysics::High Energy Astrophysical PhenomenaNumerical analysissymbolsRiemann solver
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A Numerical Study of Relativistic Jets

1996

Numerical simulations of supersonic jets are able to explain the structures observed in many VLA images of radio sources. The improvements achieved in classical simulations (see Hardee, these proceedings) are in contrast with the almost complete lack of relativistic simulations the reason being that numerical difficulties arise from the highly relativistic flows typical of extragalactic jets. For our study, we have developed a two-dimensional code which is based on (i) an explicit conservative differencing of the special relativistic hydrodynamics (SRH) equations and (ii) the use of an approximate Riemann solver (see Marti et al. 1995a,b and references therein).

PhysicsCode (set theory)symbols.namesakeAstrophysical jetAstrophysics::High Energy Astrophysical PhenomenasymbolsSupersonic speedRiemann solverComputational physics
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