Numerical model for the evolution of a supernova remnant

Details Numerical model for the evolution of a supernova remnant Numerical model for the evolution of a supernova remnant

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48...41f&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, Mar. 1977, p. 41-53. In Italian.

Astronomy and Astrophysics

Astronomy

2

Energy Conservation, Hydrodynamic Equations, Numerical Integration, Shock Wave Propagation, Supernova Remnants, Equations Of Motion, Phase Error, Radiative Heat Transfer, Similarity Theorem

Scientific paper

The paper proposes a model which enables the numerical integration of the equations of motion of a shock wave generated in a supernova explosion in a medium of uniform density. The integration method confirms energy conservation with an error of 0.2 percent in phase II of supernova-remnant evolution and with an error less than 1 percent in phase III, where the effects of radiative cooling predominate. Phase IV of evolution is also considered.

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