Boosting the accuracy of SPH techniques: Newtonian and special-relativistic tests
arXiv:1405.6034 · doi:10.1093/mnras/stv225
Abstract
We study the impact of different discretization choices on the accuracy of SPH and we explore them in a large number of Newtonian and special-relativistic benchmark tests. As a first improvement, we explore a gradient prescription that requires the (analytical) inversion of a small matrix. For a regular particle distribution this improves gradient accuracies by approximately ten orders of magnitude and the SPH formulations with this gradient outperform the standard approach in all benchmark tests. Second, we demonstrate that a simple change of the kernel function can substantially increase the accuracy of an SPH scheme. While the "standard" cubic spline kernel generally performs poorly, the best overall performance is found for a high-order Wendland kernel which allows for only very little velocity noise and enforces a very regular particle distribution, even in highly dynamical tests. Third, we explore new SPH volume elements that enhance the treatment of fluid instabilities and, last, but not least, we design new dissipation triggers. They switch on near shocks and in regions where the flow --without dissipation-- starts to become noisy. The resulting new SPH formulation yields excellent results even in challenging tests where standard techniques fail completely.
arXiv commentaccepted for publication in MNRAS
References in corpus (44)
- The cosmological simulation code GADGET-2
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Athena: A New Code for Astrophysical MHD
- Improving convergence in smoothed particle hydrodynamics simulations without pairing instability
- Smoothed Particle Hydrodynamics and Magnetohydrodynamics
- Fundamental differences between SPH and grid methods
- Rotating Stars in Relativity
- The Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation
- A General Class of Lagrangian Smoothed Particle Hydrodynamics Methods and Implications for Fluid Mixing Problems
- Smoothed Particle Hydrodynamics in Astrophysics
- Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH
- Turbulent gas motions in galaxy cluster simulations: The role of SPH viscosity
- Moving mesh cosmology: tracing cosmological gas accretion
- An energy-conserving formalism for adaptive gravitational force softening in SPH and N-body codes
- Inviscid SPH
- Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver
- An HLLC Riemann Solver for Relativistic Flows: I. Hydrodynamics
- An efficient shock-capturing central-type scheme for multidimensional relativistic flows. I. Hydrodynamics
- GENESIS: A high-resolution code for 3D relativistic hydrodynamics
- A Density Independent Formulation of Smoothed Particle Hydrodynamics
- Astrophysical Smooth Particle Hydrodynamics
- Subsonic turbulence in smoothed particle hydrodynamics and moving-mesh simulations
- Resolving mixing in Smoothed Particle Hydrodynamics
- Moving mesh cosmology: the hydrodynamics of galaxy formation
- SPHS: Smoothed Particle Hydrodynamics with a higher order dissipation switch
- TESS: A Relativistic Hydrodynamics Code on a Moving Voronoi Mesh
- MAGMA: a 3D, Lagrangian magnetohydrodynamics code for merger applications
- Moving Mesh Cosmology: Properties of Gas Disks
- Computational Eulerian Hydrodynamics and Galilean Invariance
- Particle hydrodynamics with tessellation techniques
- A one-parameter family of interpolating kernels for Smoothed Particle Hydrodynamics studies
- VINE -- A numerical code for simulating astrophysical systems using particles I: Description of the physics and the numerical methods
- rpSPH: a novel Smoothed Particle Hydrodynamics Algorithm
- Improving smoothed particle hydrodynamics with an integral approach to calculating gradients
- Kelvin-Helmholtz instabilities with Godunov SPH
- Moving mesh cosmology: properties of neutral hydrogen in absorption
- Conservative, special-relativistic smoothed particle hydrodynamics
- Numerical overcooling in shocks
- Hydrodynamic simulations with the Godunov SPH
- The Relative Stability Against Merger of Close, Compact Binaries
- Kelvin-Helmholtz instabilities in Smoothed Particle Hydrodynamics
- Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
- Hydrodynamic capabilities of an SPH code incorporating an artificial conductivity term with a gravity-based signal velocity
- Testing the concept of integral approach to derivatives within the smoothed particle hydrodynamics technique in astrophysical scenarios
Cited by in corpus (54)
- Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
- Gasoline2: A Modern SPH Code
- Accurate, Meshless Methods for Magneto-Hydrodynamics
- Detectability of compact binary merger macronovae
- Anisotropic Diffusion in Mesh-Free Numerical Magnetohydrodynamics
- Magnetohydrodynamical simulations of a tidal disruption in general relativity
- CRKSPH - A Conservative Reproducing Kernel Smoothed Particle Hydrodynamics Scheme
- An advanced leakage scheme for neutrino treatment in astrophysical simulations
- Seeding the Second Star: enrichment from population III, dust evolution, and cloud collapse
- Collision velocity of dust grains in self-gravitating protoplanetary discs
- DISCO: A 3D Moving-Mesh Magnetohydrodynamics Code Designed for the Study of Astrophysical Disks
- GANDALF - Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids
- Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
- Protoplanetary Disc Response to Distant Tidal Encounters in Stellar Clusters
- Smoothed particle hydrodynamics simulations of gas and dust mixtures
- The Lagrangian hydrodynamics code MAGMA2
- SPHYNX: an accurate density-based SPH method for astrophysical applications
- Enhanced mixing in giant impact simulations with a new Lagrangian method
- Local simulations of MRI turbulence with meshless methods
- SPH/N-body simulations of small (D = 10 km) asteroidal breakups and improved parametric relations for Monte-Carlo collisional models
- SPHINCS_BSSN: A general relativistic Smooth Particle Hydrodynamics code for dynamical spacetimes
- A multifiltering study of turbulence in a large sample of simulated galaxy clusters
- Parametric instability in a free evolving warped protoplanetary disc
- A study of cool core resiliency and entropy mixing in simulations of galaxy cluster mergers
- Santa Barbara Cluster Comparison Test with DISPH
- A comparison of SPH artificial viscosities and their impact on the Keplerian disk
- Improved Performances in Subsonic Flows of an SPH Scheme with Gradients Estimated using an Integral Approach
- Techniques for second order convergent weakly-compressible smoothed particle hydrodynamics schemes without boundaries
- Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
- A simple, entropy-based dissipation trigger for SPH
- Simulating neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN
- Light Curves and Spectra from a Unimodal Core-Collapse SuperNova
- Calibration of the Advanced Spectral Leakage scheme for neutron star merger simulations, and extension to smoothed-particle hydrodynamics
- Smoothed particle magnetohydrodynamics with the geometric density average force expression
- Finding Neighbors in a Forest: A b-tree for Smoothed Particle Hydrodynamics Simulations
- Conservative, density-based smoothed particle hydrodynamics with improved partition of the unity and better estimation of gradients
- Equalizing resolution in smoothed-particle hydrodynamics calculations using self-adaptive sinc kernels
- REMIX SPH -- improving mixing in smoothed particle hydrodynamics simulations using a generalised, material-independent approach
- Dust accretion in binary systems: implications for planets and transition discs
- Smoothed Particle Hydrodynamics with Smoothed Pseudo-Density
- Sub-stellar engulfment by a main sequence star: where is the lithium?
- The Lagrangian Numerical Relativity code SPHINCS_BSSN_v1.0
- An improved SPH scheme for cosmological simulations
- Axisymmetric smoothed particle magneto-hydrodynamics
- Adaptive Compressible Smoothed Particle Hydrodynamics
- SPH Methods in the Modelling of Compact Objects
- Modeling Solids in Nuclear Astrophysics with Smoothed Particle Hydrodynamics
- Detection of Silent Data Corruptions in Smoothed Particle Hydrodynamics Simulations
- Halted-Pendulum Relaxation: Application to White Dwarf Binary Initial Data
- Mixing Sinc kernels to improve interpolations in smoothed particle hydrodynamics without pairing instability
- Towards a Mini-App for Smoothed Particle Hydrodynamics at Exascale
- Nonlinear behaviour of warped discs around a central object with a quadrupole moment
- Optimized smoothing kernels for SPH
- Shock-capturing particle hydrodynamics with reproducing kernels