Propagation of discontinuities in a hot relativistic plasma in intense magnetic fields

Physics – Plasma Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

High Temperature Plasmas, Magnetoplasmadynamics, Relativistic Plasmas, Shock Discontinuity, Stellar Magnetic Fields, Compression Waves, Cosmic Plasma, Hyperspaces, Magnetohydrodynamic Waves, Plasma Physics, Propagation Modes, Radiation Pressure, Shock Wave Interaction, Shock Wave Propagation, Wave Propagation, Weak Energy Interactions

Scientific paper

The problem of growth and decay of weak waves in relativistic hot plasma in intense magnetic fields is investigated by using the singular surface theory, and the amplitude of the critical stage is determined when the weak wave breaks down and a shock wave forms due to nonlinear steepening. The weak wave or weak discontinuity is studied in the form of a time-like singular hypersurface across which flow parameters are continuous except for their first and higher partial derivatives which undergo finite jumps at the surface. Modes of propagation are analyzed using compatibility conditions for the jumps of inner parts of equations governing the motion of a relativistic thermodynamically perfect radiating magnetofluid of infinite electrical conductivity with a constant magnetic permeability. The effects of wave geometry on the global behavior of the amplitude are also examined.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Propagation of discontinuities in a hot relativistic plasma in intense magnetic fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Propagation of discontinuities in a hot relativistic plasma in intense magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Propagation of discontinuities in a hot relativistic plasma in intense magnetic fields will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1018340

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.