Simulation of the Magnetorotational Supernova Explosion Mechanism.

Details Simulation of the Magnetorotational Supernova Explosion Mechanism. Simulation of the Magnetorotational Supernova Explosion Mechanism.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.460m&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results of 2D simulation of the magnetorotational supernova explosion. Simulation has been done using implicit Lagrangian scheme on triangular grig with grid reconstruction. Amplification of the toroidal magnetic field due to the differential rotation in the star leads to the formation of the of compression wave moving outwars. This wave transforms to the shock wave and ejects part of the envelope. Time evolution of the amount of the ejected mass and ejected energy are given.

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