论文标题

Sphenix:平滑的粒子流体动力学,用于下一代星系模拟

Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations

论文作者

Borrow, Josh, Schaller, Matthieu, Bower, Richard G., Schaye, Joop

论文摘要

平滑的颗粒流体动力学(SPH)是一种无处不在的数值方法,用于求解流体方程,并以其保护特性,自然适应性和简单性而受到珍视。我们介绍了SPHENIX SPH方案,该方案的设计有三个关键目标:与注入能量的子网格物理模块很好地合作,在计算和内存方面都非常有效(无论是计算和内存而言),并且是Lagrangian。 SPHENIX使用一个密度 - 能量运动方程,以及可变的人工粘度和传导,包括旨在与星系形成的常见子网格模型一起使用的限制器。特别是,我们提出并测试一个新的限制器,可防止跨冲击传导,从而防止反馈事件中的虚假辐射损失。 Sphenix被证明可以解决传统SPH的许多困难测试问题,包括流体混合和涡度保护,并且显示在适当的所有测试中都会产生收敛行为。至关重要的是,我们将SPHENIX中的各种开关都使用相同的参数,以证明该方案的性能,因为它将用于生产模拟。

Smoothed Particle Hydrodynamics (SPH) is a ubiquitous numerical method for solving the fluid equations, and is prized for its conservation properties, natural adaptivity, and simplicity. We introduce the Sphenix SPH scheme, which was designed with three key goals in mind: to work well with sub-grid physics modules that inject energy, be highly computationally efficient (both in terms of compute and memory), and to be Lagrangian. Sphenix uses a Density-Energy equation of motion, along with variable artificial viscosity and conduction, including limiters designed to work with common sub-grid models of galaxy formation. In particular, we present and test a novel limiter that prevents conduction across shocks, preventing spurious radiative losses in feedback events. Sphenix is shown to solve many difficult test problems for traditional SPH, including fluid mixing and vorticity conservation, and it is shown to produce convergent behaviour in all tests where this is appropriate. Crucially, we use the same parameters within Sphenix for the various switches throughout, to demonstrate the performance of the scheme as it would be used in production simulations.

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