2008/02/29 by Z. Osmanov, A. Mignone, S. Massaglia +2
Engineering · Mathematics · Physics and Astronomy · #Boundary value problem #Classical mechanics #Cosmology and Gravitation Theories #Fluid Dynamics and Turbulent Flows #Geometry #Helmholtz equation #Helmholtz free energy #High-Energy Particle Collisions Research #Instability #Linear stability #Magnetohydrodynamic drive #Magnetohydrodynamics #Mathematics #Mechanics #Motion (physics) #Physics #Planar #Plane (geometry) #Plasma #Quantum mechanics #Stability (learning theory) #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809605
8 pages, 9 figures
arxiv created 2008/08/14 · openalex publication_date 2008/09/11 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. We investigate the linear stability properties of the plane interface separating two relativistic magnetized flows in motion with respect to each other. The two flows are governed by the (special) relativistic equations for a magnetized perfect gas in the infinite conductivity approximation.