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Different magneto-rotational supernovae

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Abstract

We present the results of two-dimensional calculations of a magneto-rotational (MR) supernova explosion with a collapsing core for various core masses, rotational angular momenta, and magnetic-field configurations. It is shown that the MR mechanism produces an explosion energy that corresponds to observed values. The form of the explosion depends substantially on the initial configuration of the magnetic field. MR instability develops during the evolution of the magnetic field in an MR supernova explosion, resulting in an exponential increase of all components of the magnetic field, thereby substantially decreasing the time scale of the MR explosion. The energy of the supernova increases with the core’s mass and initial rotational energy.

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Authors and Affiliations

  1. Space Research Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, GSP-7, Moscow, 117810, Russia

    G. S. Bisnovatyi-Kogan & S. G. Moiseenko

  2. Moscow State University, Moscow, 119899, Russia

    N. V. Ardelyan

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  1. G. S. Bisnovatyi-Kogan
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  2. S. G. Moiseenko
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  3. N. V. Ardelyan
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Original Russian Text © G.S. Bisnovatyi-Kogan, S.G. Moiseenko, N.V. Ardelyan, 2008, published in Astronomicheskiĭ Zhurnal, 2008, Vol. 85, No. 12, pp. 1109–1121.

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Bisnovatyi-Kogan, G.S., Moiseenko, S.G. & Ardelyan, N.V. Different magneto-rotational supernovae. Astron. Rep. 52, 997–1008 (2008). https://doi.org/10.1134/S1063772908120056

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  • DOI: https://doi.org/10.1134/S1063772908120056

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