School of Science
Department of Physics
18309
18309 Plasma Astrophysics
Course Webpage: https://eclass.uoa.gr/courses/PHYS345/
Course Content
- Steady magnetized flows with an ignorable coordinate. Magnetohydrodynamic (MHD) waves (Alfvèn, fast and slow magnetosonic waves).
- Magnetized winds and angular momentum extraction in young stellar objects, Weber-Davis model.
- Jeans gravitational instability. Star formation, angular momentum, magnetic flux and efficiency problems, evolution of stellar rotation, magnetic critical collapse mass, Skumanich's law.
- Astrophysical jets. Minimum inclination of outflow fieldlines with respect to the axis of rotation. Collimation of MHD outflows and examples.
- Self-similarity. Families of models for describing self-similar MHD jets. Critical points, separatrix surfaces and causality in MHD outflows. Collimation criteria.
- Method of characteristics (steady supersonic flow, Riemann invariants). Magnetohydrodynamic shock waves. Magnetic dynamo. Magnetic reconnection.
- Relativistic magnetohydrodynamics, applications to γ-ray bursts and jets from active galactic nuclei.
- Instabilities (Rayleigh-Taylor, Kelvin-Helmholtz, pinch, kink, Parker, magnetorotational).
- Kinetic theory for collisionless magnetized plasmas. Plasma oscillations and Landau damping.