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pro vyhledávání: '"Herrmann, Hans J."'
Publikováno v:
ESAIM: Proceedings and Surveys, Vol 52, Pp 66-75 (2015)
We provide numerical evidence that the Richtmyer-Meshkov (RM) instability contributes to the cooling of a relativistic fluid. Due to the presence of jet particles traveling throughout the medium, shock waves are generated in the form of Mach cones.
Externí odkaz:
https://doaj.org/article/d5172aebc2994e3297ed62a1ddd160ce