Neutrino fluxes from a core-collapse supernova in a model with three sterile neutrinos


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The characteristics of the gravitational collapse of a supernova and the fluxes of active and sterile neutrinos produced during the formation of its protoneutron core have been calculated numerically. The relative yields of active and sterile neutrinos in corematter with different degrees of neutronization have been calculated for various input parameters and various initial conditions. A significant increase in the fraction of sterile neutrinos produced in superdense core matter at the resonant degree of neutronization has been confirmed. The contributions of sterile neutrinos to the collapse dynamics and the total flux of neutrinos produced during collapse have been shown to be relatively small. The total luminosity of sterile neutrinos is considerably lower than the luminosity of electron neutrinos, but their spectrum is considerably harder at high energies.

作者简介

A. Yudin

Institute for Theoretical and Experimental Physics

编辑信件的主要联系方式.
Email: yudin@itep.ru
俄罗斯联邦, ul. Bol’shaya Cheremushkinskaya 25, Moscow, 117218

D. Nadyozhin

Institute for Theoretical and Experimental Physics; “Kurchatov Institute” National Research Center

Email: yudin@itep.ru
俄罗斯联邦, ul. Bol’shaya Cheremushkinskaya 25, Moscow, 117218; pl. Kurchatova 1, Moscow, 123182

V. Khruschov

“Kurchatov Institute” National Research Center; Center for Gravitation and Fundamental Metrology

Email: yudin@itep.ru
俄罗斯联邦, pl. Kurchatova 1, Moscow, 123182; ul. Ozernaya 46, Moscow, 119361

S. Fomichev

“Kurchatov Institute” National Research Center; Moscow Institute of Physics and Technology

Email: yudin@itep.ru
俄罗斯联邦, pl. Kurchatova 1, Moscow, 123182; Dolgoprudnyi, Moscow oblast, 141700

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