Propagation of axi-symmetric relativistic shock waves

Details Propagation of axi-symmetric relativistic shock waves Propagation of axi-symmetric relativistic shock waves

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..323r&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 2, Oct. 1980, p. 323-345.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Axisymmetric Flow, Gas Expansion, Relativity, Shock Wave Propagation, Supernovae, Explosions, Flux Density, Numerical Integration, Transformations (Mathematics), Velocity Distribution

Scientific paper

Solutions in series for the propagation of relativistic shock waves with axial symmetry are obtained in this paper. It is assumed that the gaseous elements move almost radially and that the disturbance moves through a cold gas at rest wherein the nucleon number density and the energy density obey an exponential law of distance from a given plane. The motion is sustained by continuous explosions in the central region liberating energy varying as the cube of time. Also, the equation of state of the moving elements is assumed to be that of photonic gas.

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