Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity

IF 26.3 2区 物理与天体物理 Q1 PHYSICS, PARTICLES & FIELDS
José A. Font
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引用次数: 202

Abstract

This article presents a comprehensive overview of numerical hydrodynamics and magneto-hydrodynamics (MHD) in general relativity. Some significant additions have been incorporated with respect to the previous two versions of this review (2000, 2003), most notably the coverage of general-relativistic MHD, a field in which remarkable activity and progress has occurred in the last few years. Correspondingly, the discussion of astrophysical simulations in general-relativistic hydrodynamics is enlarged to account for recent relevant advances, while those dealing with general-relativistic MHD are amply covered in this review for the first time. The basic outline of this article is nevertheless similar to its earlier versions, save for the addition of MHD-related issues throughout. Hence, different formulations of both the hydrodynamics and MHD equations are presented, with special mention of conservative and hyperbolic formulations well adapted to advanced numerical methods. A large sample of numerical approaches for solving such hyperbolic systems of equations is discussed, paying particular attention to solution procedures based on schemes exploiting the characteristic structure of the equations through linearized Riemann solvers. As previously stated, a comprehensive summary of astrophysical simulations in strong gravitational fields is also presented. These are detailed in three basic sections, namely gravitational collapse, black-hole accretion, and neutron-star evolutions; despite the boundaries, these sections may (and in fact do) overlap throughout the discussion. The material contained in these sections highlights the numerical challenges of various representative simulations. It also follows, to some extent, the chronological development of the field, concerning advances in the formulation of the gravitational field, hydrodynamics and MHD equations and the numerical methodology designed to solve them. To keep the length of this article reasonable, an effort has been made to focus on multidimensional studies, directing the interested reader to earlier versions of the review for discussions on one-dimensional works.

Abstract Image

广义相对论中的数值流体力学和磁流体力学
本文介绍了广义相对论中数值流体力学和磁流体力学(MHD)的综合概况。与本综述的前两个版本(2000年、2003年)相比,有一些重要的补充内容被纳入其中,最引人注目的是对广义相对论MHD的报道,这是一个在过去几年中发生了显著活动和进展的领域。相应的,在广义相对论流体力学中天体物理模拟的讨论被扩大,以考虑到最近的相关进展,而那些处理广义相对论MHD的讨论第一次被充分地涵盖在这篇综述中。尽管如此,本文的基本大纲与其早期版本相似,只是增加了一些与mhd相关的问题。因此,提出了流体力学和MHD方程的不同公式,特别提到了适用于先进数值方法的保守公式和双曲公式。讨论了求解这类双曲型方程组的大量数值方法,特别注意了基于利用线性化黎曼解的方程特征结构的方案的求解过程。如前所述,本文还对强引力场下的天体物理模拟进行了全面总结。这些在三个基本章节中进行了详细介绍,即引力坍缩、黑洞吸积和中子星演化;尽管有这些界限,这些部分在整个讨论中可能(事实上也确实)重叠。这些章节中包含的材料强调了各种代表性模拟的数值挑战。在某种程度上,它也遵循该领域的时间顺序发展,涉及重力场、流体力学和MHD方程的公式的进展以及为求解这些方程而设计的数值方法。为了保持本文的长度合理,我们努力将重点放在多维研究上,引导感兴趣的读者阅读本文的早期版本,以讨论一维作品。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Living Reviews in Relativity
Living Reviews in Relativity 物理-物理:粒子与场物理
CiteScore
69.90
自引率
0.70%
发文量
0
审稿时长
20 weeks
期刊介绍: Living Reviews in Relativity is a peer-reviewed, platinum open-access journal that publishes reviews of research across all areas of relativity. Directed towards the scientific community at or above the graduate-student level, articles are solicited from leading authorities and provide critical assessments of current research. They offer annotated insights into key literature and describe available resources, maintaining an up-to-date suite of high-quality reviews, thus embodying the "living" aspect of the journal's title. Serving as a valuable tool for the scientific community, Living Reviews in Relativity is often the first stop for researchers seeking information on current work in relativity. Written by experts, the reviews cite, explain, and assess the most relevant resources in a given field, evaluating existing work and suggesting areas for further research. Attracting readers from the entire relativity community, the journal is useful for graduate students conducting literature surveys, researchers seeking the latest results in unfamiliar fields, and lecturers in need of information and visual materials for presentations at all levels.
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