Propagation of cylindrical relativistic shock waves in the presence of a magnetic field

Details Propagation of cylindrical relativistic shock waves in the presence of a magnetic field Propagation of cylindrical relativistic shock waves in the presence of a magnetic field

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..61..101d&link_type=abstract

Astrophysics and Space Science, vol. 61, no. 1, Mar. 1979, p. 101-110.

Other

4

Cylindrical Waves, Magnetic Fields, Relativistic Plasmas, Shock Wave Propagation, Similarity Theorem, Cold Gas, Density Distribution, Energy Distribution, Equations Of Motion, Isothermal Flow, Nucleons, Shock Fronts, Velocity Distribution

Scientific paper

Similarity solutions for the propagation of cylindrical relativistic shock waves in the presence of a constant azimuthal magnetic field or in its absence are obtained for a medium where the nucleon number density is uniform. The shock surface moves with constant velocity, and the total energy of the disturbance is dependent on time. The solutions are applicable only to an isothermal medium or a cold gas.

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