相对论性耗散流体动力学理论
Theories of Relativistic Dissipative Fluid Dynamics.
作者信息
Rocha Gabriel S, Wagner David, Denicol Gabriel S, Noronha Jorge, Rischke Dirk H
机构信息
Department of Physics and Astronomy, Vanderbilt University, 1221 Stevenson Center Lane, Nashville, TN 37212, USA.
Instituto de Física, Universidade Federal Fluminense, 24210-346 Niterói, RJ, Brazil.
出版信息
Entropy (Basel). 2024 Feb 22;26(3):189. doi: 10.3390/e26030189.
Relativistic dissipative fluid dynamics finds widespread applications in high-energy nuclear physics and astrophysics. However, formulating a causal and stable theory of relativistic dissipative fluid dynamics is far from trivial; efforts to accomplish this reach back more than 50 years. In this review, we give an overview of the field and attempt a comparative assessment of (at least most of) the theories for relativistic dissipative fluid dynamics proposed until today and used in applications.
相对论性耗散流体动力学在高能核物理和天体物理学中有广泛应用。然而，构建一个因果性且稳定的相对论性耗散流体动力学理论绝非易事；为此所做的努力可以追溯到50多年前。在这篇综述中，我们对该领域进行概述，并尝试对迄今为止提出并应用于实际的（至少是大部分）相对论性耗散流体动力学理论进行比较评估。
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