Shock-capturing particle hydrodynamics with reproducing kernels
arXiv:2411.19228 · doi:10.32604/cmes.2025.062063
Abstract
We present and explore a new shock-capturing particle hydrodynamics approach. Our starting point is a commonly used discretization of smoothed particle hydrodynamics. We enhance this discretization with Roe's approximate Riemann solver, we identify its dissipative terms, and in these terms, we use slope-limited linear reconstruction. All gradients needed for our method are calculated with linearly reproducing kernels that are constructed to enforce the two lowest-order consistency relations. We scrutinize our reproducing kernel implementation carefully on a "glass-like" particle distribution, and we find that constant and linear functions are recovered to machine precision. We probe our method in a series of challenging 3D benchmark problems ranging from shocks over instabilities to Schulz-Rinne-type vorticity-creating shocks. All of our simulations show excellent agreement with analytic/reference solutions.
28 pages, 21 figures; accepted for publication in "Computer Modeling in Engineering and Sciences"
References in corpus (28)
- SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations
- Improving convergence in smoothed particle hydrodynamics simulations without pairing instability
- Smoothed Particle Hydrodynamics and Magnetohydrodynamics
- Fundamental differences between SPH and grid methods
- Producing ultra-strong magnetic fields in neutron star mergers
- Smoothed Particle Hydrodynamics in Astrophysics
- Inviscid SPH
- Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers
- Hydromagnetic turbulence in computer simulations
- Reformulation of Smoothed Particle Hydrodynamics with Riemann Solver
- A Density Independent Formulation of Smoothed Particle Hydrodynamics
- Astrophysical Smooth Particle Hydrodynamics
- A Well-Posed Kelvin-Helmholtz Instability Test and Comparison
- Producing Magnetar Magnetic Fields in the Merger of Binary Neutron Stars
- Astrophysical Weighted Particle Magnetohydrodynamics
- CRKSPH - A Conservative Reproducing Kernel Smoothed Particle Hydrodynamics Scheme
- Boosting the accuracy of SPH techniques: Newtonian and special-relativistic tests
- A one-parameter family of interpolating kernels for Smoothed Particle Hydrodynamics studies
- rpSPH: a novel Smoothed Particle Hydrodynamics Algorithm
- Improving smoothed particle hydrodynamics with an integral approach to calculating gradients
- DISCO: A 3D Moving-Mesh Magnetohydrodynamics Code Designed for the Study of Astrophysical Disks
- A fast recursive coordinate bisection tree for neighbour search and gravity
- The Lagrangian hydrodynamics code MAGMA2
- Testing the concept of integral approach to derivatives within the smoothed particle hydrodynamics technique in astrophysical scenarios
- A simple, entropy-based dissipation trigger for SPH
- The role of time integration in energy conservation in Smoothed Particle Hydrodynamics fluid dynamics simulations
- REMIX SPH -- improving mixing in smoothed particle hydrodynamics simulations using a generalised, material-independent approach
- The Lagrangian Numerical Relativity code SPHINCS_BSSN_v1.0