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Multigroup radiative transfer in supernova shock breakout models

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Abstract

The physical peculiarities of supernova shock breakout are discussed. A number of models for various types of supernovae have been constructed based on multigroup radiative transfer by taking these peculiarities into account. The results of numerical simulations and the influence of the effects of photon scattering by electrons and the thermalization depth on them are considered. It is shown under which conditions the appearance of hard X-ray emission is possible at shock breakout. It is pointed out what refinements are necessary in the computational algorithms for radiative transfer and hydrodynamics.

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Authors and Affiliations

  1. Institute for Theoretical and Experimental Physics, ul. Bol’shaya Cheremushkinskaya 25, Moscow, 117259, Russia

    S. I. Blinnikov & A. G. Tolstov

  2. Institute of Physics and Mathematics of the Universe, University of Tokyo, Tokyo, Japan

    S. I. Blinnikov

  3. Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992, Russia

    S. I. Blinnikov

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  1. S. I. Blinnikov
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  2. A. G. Tolstov
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Correspondence to S. I. Blinnikov.

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Original Russian Text © S.I. Blinnikov, A.G. Tolstov, 2011, published in Pis’ma v Astronomicheskiℝ Zhurnal, 2011, Vol. 37, No. 3, pp. 217–232.

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Blinnikov, S.I., Tolstov, A.G. Multigroup radiative transfer in supernova shock breakout models. Astron. Lett. 37, 194–209 (2011). https://doi.org/10.1134/S1063773711010051

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