An asymptotically correct implicit-explicit time integration scheme for finite volume radiation-hydrodynamics

被引:1
|
作者
He, Chong-Chong [1 ]
Wibking, Benjamin D. [2 ]
Krumholz, Mark R. [1 ,3 ]
机构
[1] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia
[2] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[3] ARC Ctr Excellence Astron Three Dimens ASTRO 3D, Canberra, ACT 2611, Australia
基金
澳大利亚研究理事会;
关键词
diffusion; hydrodynamics; radiation: dynamics; methods: numerical; DIFFUSION; PRESSURE; DISCRETIZATION; DISKS;
D O I
10.1093/mnras/stae1244
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Numerical radiation-hydrodynamics (RHD) for non-relativistic flows is a challenging problem because it encompasses processes acting over a very broad range of time-scales, and where the relative importance of these processes often varies by orders of magnitude across the computational domain. Here, we present a new implicit-explicit method for numerical RHD that has a number of desirable properties that have not previously been combined in a single method. Our scheme is based on moments and allows machine-precision conservation of energy and momentum, making it highly suitable for adaptive mesh refinement applications; it requires no more communication than hydrodynamics and includes no non-local iterative steps, making it highly suitable for massively parallel and Graphics Processing Unit (GPU)-based systems where communication is a bottleneck; and we show that it is asymptotically accurate in the streaming, static diffusion, and dynamic diffusion limits, including in the so-called asymptotic diffusion regime where the computational grid does not resolve the photon mean-free path. We implement our method in the GPU-accelerated RHD code quokka and show that it passes a wide range of numerical tests.
引用
收藏
页码:1228 / 1242
页数:15
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