Novel hydrodynamic schemes capturing shocks and contact discontinuities and comparison study with existing methods
arXiv:2312.03224Publication · DOI
Approach
Several formulations are compared with existing SPH schemes using Riemann, pressure-equilibrium, Sedov–Taylor and Kelvin–Helmholtz tests.
Main result
Two GDISPH variants perform well on shocks and contact discontinuities. Case 1 offers the preferred balance without manually selected viscosity parameters or added numerical diffusion.
Scientific implications
The method addresses numerical surface tension and shock handling, both central to simulations of multiphase astrophysical gas.
Scope and limitations
The comparative advantage is established on the reported benchmark suite; performance in a specific galaxy simulation still depends on its physical and numerical setup.