Dissipation process of binary mixture gas in thermally relativistic flow
Ryosuke Yano

TL;DR
This paper investigates the dissipation process of binary mixture gases in relativistic flows, focusing on diffusion flux characteristics, comparing relativistic Boltzmann equation results with NSF approximations, and emphasizing the importance of particle four flow for accuracy.
Contribution
It provides a detailed analysis of diffusion flux in relativistic binary gases, highlighting limitations of NSF approximation and proposing the use of particle four flow for precise calculation.
Findings
Diffusion flux near walls differs significantly from NSF approximation.
Diffusion flux inside shock wave aligns with NSF approximation.
Accurate diffusion flux calculation requires particle four flow.
Abstract
In this paper, we discuss dissipation process of the binary mixture gas in the thermally relativistic flow \textcolor{red}{by focusing on the characteristics of the diffusion flux}. As an analytical object, we consider the relativistic rarefied-shock layer problem around the triangle prism. Numerical results of the diffusion flux are compared with the Navier-Stokes-Fourier (NSF) order approximation of the diffusion flux, which is calculated using the diffusion and thermal-diffusion coefficients by Kox \textit{et al}. [Physica A, 84, 1, pp.165-174 (1976)]. In the case of the uniform flow with the small Lorentz contraction, the diffusion flux, which is obtained by calculating the relativistic Boltzmann equation, is roughly approximated by the NSF order approximation inside the shock wave, whereas the diffusion flux in the vicinity of the wall is markedly different from the NSF order…
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