Heat conduction in relativistic systems: alternatives and perspectives
C. S. Lopez-Monsalvo

TL;DR
This paper reviews approaches to modeling heat conduction in relativistic systems, emphasizing the multi-fluid method, and discusses the phenomenology of relativistic dissipation in non-equilibrium thermodynamics.
Contribution
It provides a concise overview of the multi-fluid approach to relativistic heat conduction and explores alternative perspectives in relativistic dissipation modeling.
Findings
Highlights the complexity of relativistic heat conduction phenomenology
Summarizes efforts and methods in relativistic dissipation modeling
Emphasizes the potential of multi-fluid approaches
Abstract
The non-equilibrium thermodynamics of relativistic systems have a rich phenomenology. The simplest phenomenon in the class of dissipative processes is that of heat. This letter presents a brief summary of the efforts made to tackle the problem of relativistic heat conduction. In particular, we focus on the multi-fluid approach to relativistic dissipation.
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Taxonomy
TopicsHigh-pressure geophysics and materials · Gas Dynamics and Kinetic Theory · Pulsars and Gravitational Waves Research
