Hybrid radiation hydrodynamics scheme with adaptive gravity-tree-based pseudo-particles
Cheryl S. C. Lau, Maya A. Petkova, Ian A. Bonnell

TL;DR
This paper introduces an optimized hybrid radiation hydrodynamics scheme that adaptively simplifies fluid representations using pseudo-particles, significantly improving computational efficiency while maintaining accuracy in astrophysical simulations.
Contribution
The authors develop a novel adaptive method converting gravity tree nodes into pseudo-SPH particles, reducing computational load in hybrid RHD simulations.
Findings
Achieves strong agreement with benchmark results.
Provides significant speed-up in simulations.
Maintains accuracy with adaptive pseudo-particle approach.
Abstract
HII regions powered by ionizing radiation from massive stars drive the dynamical evolution of the interstellar medium. Fast radiative transfer methods for incorporating photoionization effects are thus essential in astrophysical simulations. Previous work by Petkova et al. established a hybrid radiation hydrodynamics (RHD) scheme that couples Smoothed Particle Hydrodynamics (SPH) to grid-based Monte Carlo Radiative Transfer (MCRT) code. This particle-mesh scheme employs the Exact mapping method for transferring fluid properties between SPH particles and Voronoi grids on which the MCRT simulation is carried out. The mapping, however, can become computationally infeasible with large numbers of particles or grid cells. We present a novel optimization method that adaptively converts gravity tree nodes into pseudo-SPH particles. These pseudo-particles act in place of the SPH particles when…
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Taxonomy
TopicsFluid Dynamics Simulations and Interactions · Fluid Dynamics and Heat Transfer · Lattice Boltzmann Simulation Studies
