The motion of the cylindrical symmetrical relativistic shock wave in the presence of an axial magnetic field

Details The motion of the cylindrical symmetrical relativistic shock wave in the presence of an axial magnetic field The motion of the cylindrical symmetrical relativistic shock wave in the presence of an axial magnetic field

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.125..379c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 125, no. 2, Aug. 1986, p. 379-390.

Statistics

Computation

Computational Astrophysics, Magnetic Effects, Relativistic Effects, Shock Waves, Supernovae, Propagation Velocity, Similarity Theorem

Scientific paper

The motion of a special relativistic shock wave which propagates from the center line outwards after an explosion is considered under the assumption that the magnetic field consists of only an axial component. Similarity solutions which depend on the parameter zeta = r/t are found to exist. The cases of an ultrarelativistic fluid in front of the shock, and of a cold fluid in front of the shock, are examined in detail. Numerical results are presented.

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