On the mode structure of imperfect fluids
DOI:
https://doi.org/10.47456/Cad.Astro.v3n1.36856Palabras clave:
Causal thermodynamics, long-wavelength perturbation modesResumen
This paper tries to present a simple picture of several aspects of the mode structure in relativistic non-equilibrium thermodynamics. Its pedagogical focus is on the relation between long-wavelength perturbation modes of the causal Müller-Israel-Stewart (MIS) theory and those of the traditional Eckart theory. Principally, this issue was clarified in a series of papers by Hiscock and Lindblom. Here, I put together some essential features of this topic which do not require the entire formalism of the complete theory.
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Derechos de autor 2022 Winfried Zimdahl
Esta obra está bajo una licencia internacional Creative Commons Atribución 4.0.