Special Relativistic Smoothed Particle Hydrodynamics Based on Riemann Solver
Kanta Kitajima, Shu-ichiro Inutsuka, Izumi Seno
TL;DR
The paper addresses accurate simulation of special-relativistic hydrodynamics with SPH and introduces SRGSPH, a Godunov-based SPH framework that leverages a Riemann solver for inter-particle fluxes and convolution-based field estimates to enhance shock capturing. It also proposes a volume-based density definition and a variable smoothing-length scheme to handle nonuniform baryon numbers while preserving conservation properties. The method is validated through a comprehensive suite of one- and two-dimensional shock-tube problems and Kelvin-Helmholtz instability tests, demonstrating robust accuracy and smooth handling of density variations. The results indicate that SRGSPH offers improved resolution of shocks and discontinuities in relativistic flows, with potential extensions to general-relativistic hydrodynamics for high-energy astrophysical applications.
Abstract
This paper proposes a novel numerical method based on Godunov Smoothed Particle Hydrodynamics for special relativistic fluid dynamics. Our method utilizes a Riemann solver to describe shock, enhancing accuracy in strong shock waves. The formulation maintains conservation laws and achieves higher accuracy through convolution integrals that define physical quantities for SPH particles. We also propose the number density calculation method that uses a non-equal baryon number in each SPH particle and variable smoothing length in a way different from the conventional method. Numerical experiments demonstrate the method's robustness across one- and two-dimensional relativistic shock tube problems, as well as its ability to simulate Kelvin-Helmholtz instabilities accurately, validating SRGSPH as a reliable approach for high-resolution relativistic simulations.
