Improved Performances in Subsonic Flows of an SPH Scheme with Gradients Estimated using an Integral Approach
arXiv:1608.08361 · doi:10.3847/0004-637X/831/1/103
Abstract
In this paper we present results from a series of hydrodynamical tests aimed at validating the performance of a smoothed particle hydrodynamics (SPH) formulation in which gradients are derived from an integral approach. We specifically investigate the code behavior with subsonic flows, where it is well known that zeroth-order inconsistencies present in standard SPH make it particularly problematic to correctly model the fluid dynamics. In particular we consider the Gresho-Chan vortex problem, the growth of Kelvin-Helmholtz instabilities, the statistics of driven subsonic turbulence and the cold Keplerian disc problem. We compare simulation results for the different tests with those obtained, for the same initial conditions, using standard SPH. We also compare the results with the corresponding ones obtained previously with other numerical methods, such as codes based on a moving-mesh scheme or Godunov-type Lagrangian meshless methods. We quantify code performances by introducing error norms and spectral properties of the particle distribution, in a way similar to what was done in other works. We find that the new SPH formulation exhibits strongly reduced gradient errors and outperforms standard SPH in all of the tests considered. In fact, in terms of accuracy we find good agreement between the simulation results of the new scheme and those produced using other recently proposed numerical schemes. These findings suggest that the proposed method can be successfully applied for many astrophysical problems in which the presence of subsonic flows previously limited the use of SPH, with the new scheme now being competitive in these regimes with other numerical methods.
arXiv comment25 pages, 11 figures, accepted for publication in ApJ
References in corpus (49)
- The cosmological simulation code GADGET-2
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
- GIZMO: A New Class of Accurate, Mesh-Free Hydrodynamic Simulation Methods
- Athena: A New Code for Astrophysical MHD
- Cosmological SPH simulations: The entropy equation
- Enzo: An Adaptive Mesh Refinement Code for Astrophysics
- Improving convergence in smoothed particle hydrodynamics simulations without pairing instability
- Smoothed Particle Hydrodynamics and Magnetohydrodynamics
- Gasoline: An adaptable implementation of TreeSPH
- Adaptive Refinement Tree - a new high-resolution N-body code for cosmological simulations
- Fundamental differences between SPH and grid methods
- A General Class of Lagrangian Smoothed Particle Hydrodynamics Methods and Implications for Fluid Mixing Problems
- Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH
- Improving the convergence properties of the moving-mesh code AREPO
- Inviscid SPH
- Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver
- A Density Independent Formulation of Smoothed Particle Hydrodynamics
- Astrophysical Smooth Particle Hydrodynamics
- Multiphase Smoothed-Particle Hydrodynamics
- Subsonic turbulence in smoothed particle hydrodynamics and moving-mesh simulations
- Resolving mixing in Smoothed Particle Hydrodynamics
- A test suite for quantitative comparison of hydrodynamics codes in astrophysics
- SPHS: Smoothed Particle Hydrodynamics with a higher order dissipation switch
- SPHGal: Smoothed Particle Hydrodynamics with improved accuracy for Galaxy simulations
- A Well-Posed Kelvin-Helmholtz Instability Test and Comparison
- On the Origin of Cores in Simulated Galaxy Clusters
- TESS: A Relativistic Hydrodynamics Code on a Moving Voronoi Mesh
- A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence
- Numerical Convergence in Smoothed Particle Hydrodynamics
- Computational Eulerian Hydrodynamics and Galilean Invariance
- Boosting the accuracy of SPH techniques: Newtonian and special-relativistic tests
- New numerical solver for flows at various Mach numbers
- Particle hydrodynamics with tessellation techniques
- Cosmological Adaptive Mesh Refinement
- rpSPH: a novel Smoothed Particle Hydrodynamics Algorithm
- Improving smoothed particle hydrodynamics with an integral approach to calculating gradients
- Astrophysical hydrodynamics with a high-order discontinuous Galerkin scheme and adaptive mesh refinement
- Kelvin-Helmholtz instabilities with Godunov SPH
- Calibrating an updated SPH scheme within GCD+
- Hydrodynamic simulations with the Godunov SPH
- Resolving high Reynolds numbers in SPH simulations of subsonic turbulence
- The impact of numerical viscosity in SPH simulations of galaxy clusters
- Kelvin-Helmholtz instabilities in Smoothed Particle Hydrodynamics
- Modelling Shear Flows with SPH and Grid Based Methods
- Hydrodynamic capabilities of an SPH code incorporating an artificial conductivity term with a gravity-based signal velocity
- The role of the artificial conductivity in SPH simulations of galaxy clusters: effects on the ICM properties
- A comparison of SPH artificial viscosities and their impact on the Keplerian disk
- Equalizing resolution in smoothed-particle hydrodynamics calculations using self-adaptive sinc kernels
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