Theories of Relativistic Dissipative Fluid Dynamics

Entropy (Basel). 2024 Feb 22;26(3):189. doi: 10.3390/e26030189.

Abstract

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.

Keywords: fluid dynamics; kinetic theory; relativistic.

Publication types

  • Review

Grants and funding

J.N. is partially supported by the U.S. Department of Energy, Office of Science, Office for Nuclear Physics under Award DE-SC0023861. This research was partly supported by the National Science Foundation under Grant No. NSF PHY-1748958. G.S.R. is supported in part by the U.S. Department of Energy, Office of Science under Award Number DE-SC-0024347, by Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) Finance code 001, award No. 88881.650299/2021-01 and by Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), grant No. 142548/2019-7. D.W. acknowledges support by the Ministry of Research, Innovation and Digitization, CNCS - UEFISCDI, project number PN-III-P1-1.1-TE-2021-1707, within PNCDI III. D.W. and D.H.R. are supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through the CRC-TR 211 “Strong-interaction matter under extreme conditions”—project number 315477589–TRR 211, and by the State of Hesse within the Research Cluster ELEMENTS (Project ID 500/10.006).