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Magnetorotational Supernova Neutrino Emission Spectra and Prospects for Observations by Large-Size Underwater Telescopes

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Abstract

We analyze neutrino fluxes near the surface of a protoneutron star in type II supernova explosions. For magnetorotational explosion mechanism it is shown that effective neutrino collisions in a magnetized nucleon gas caused by the neutral current Gamow–Teller component lead to neutrino acceleration. Such an effect originates from spin-projection asymmetry in phase space volume of outer channel neutrino due to nucleon magnetic moment interaction with magnetic field. Respective increase in a hardness of the energy spectrum is favorable for observations of supernova neutrinos using neutrino telescopes. The possibilities of detecting supernova neutrinos by large-volume Cherenkov observatories—KM3NeT and Baikal-GVD—are discussed. As is demonstrated the upper limits of the distance thresholds for such observations can be increased by a factor of \((1.5\sqrt{k}-1/4)\), when employing the \(k\)-fold coincidence technique in data processing.

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This work was supported by ongoing institutional funding. No additional grants to carry out or direct this particular research were obtained.

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Authors and Affiliations

  1. Bogoliubov Laboratory of Theoretical Physics, JINR, Dubna, Moscow oblast, Russia

    V. N. Kondratyev

  2. Dubna State University, Dubna, Moscow oblast, Russia

    V. N. Kondratyev

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  1. V. N. Kondratyev
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Correspondence to V. N. Kondratyev.

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Kondratyev, V.N. Magnetorotational Supernova Neutrino Emission Spectra and Prospects for Observations by Large-Size Underwater Telescopes. Phys. Atom. Nuclei 86, 1083–1089 (2023). https://doi.org/10.1134/S106377882401023X

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  • DOI: https://doi.org/10.1134/S106377882401023X

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