Influence of internal energy on the stability of relativistic flows
classification
🌌 astro-ph
keywords
energyinternalstabilityinfluencejetsrelativisticamplitudeappear
read the original abstract
A set of simulations concerning the influence of internal energy on the stability of relativistic jets is presented. Results show that perturbations saturate when the amplitude of the velocity perturbation approaches the speed of light limit. Also, contrary to what predicted by linear stability theory, jets with higher specific internal energy appear to be more stable.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.