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Large-scale Instability during Gravitational Collapse with Neutrino Transport and a Core-Collapse Supernova

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Abstract

Most of the energy released in the gravitational collapse of the cores of massive stars is carried away by neutrinos. Neutrinos play a pivotal role in explaining core-collape supernovae. Currently, mathematical models of the gravitational collapse are based on multi-dimensional gas dynamics and thermonuclear reactions, while neutrino transport is considered in a simplified way. Multidimensional gas dynamics is used with neutrino transport in the flux-limited diffusion approximation to study the role of multi-dimensional effects. The possibility of large-scale convection is discussed, which is interesting both for explaining SN II and for setting up observations to register possible high-energy (≳10MeV) neutrinos from the supernova. A new multi-dimensional, multi-temperature gas dynamics method with neutrino transport is presented.

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Authors and Affiliations

  1. Institute for Computer Aided Design, Russian Academy of Sciences, 2-aya Brestskaya ul. 19/18, Moscow, 123067, Russia

    A. G. Aksenov & V. M. Chechetkin

  2. Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Miusskaya pl. 4, Moscow, 125047, Russia

    V. M. Chechetkin

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  1. A. G. Aksenov
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  2. V. M. Chechetkin
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Correspondence to A. G. Aksenov.

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Original Russian Text © A.G. Aksenov, V.M. Chechetkin, 2018, published in Astronomicheskii Zhurnal, 2018, Vol. 95, No. 4, pp. 267–279.

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Aksenov, A.G., Chechetkin, V.M. Large-scale Instability during Gravitational Collapse with Neutrino Transport and a Core-Collapse Supernova. Astron. Rep. 62, 251–263 (2018). https://doi.org/10.1134/S1063772918040017

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