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Right-polarized neutral (anti)leptons in the solar neutrino flux

  • Proceedings of the International Conference “Nuclei, 2014: Fundamental Problems of Nuclear Physics, Atomic Energy, and Nuclear Technologies” (LXIV International Meeting on Nuclear Spectroscopy and the Structure of Atomic Nuclei)
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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The flavor structure of solar beryllium neutrinos is investigated. The possible presence of neutral (anti)leptons of the second and third generations and related (electron) antineutrinos in the solar neutrino flux is considered. The energy spectra of recoil electrons upon (anti)neutrino–electron scattering are analyzed using the standard electroweak model (SM).

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References

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Authors and Affiliations

  1. Moscow State University of Design and Technology, Moscow, 117997, Russia

    Yu. I. Romanov

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  1. Yu. I. Romanov
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Correspondence to Yu. I. Romanov.

Additional information

Original Russian Text © Yu.I. Romanov, 2015, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2015, Vol. 79, No. 7, pp. 1058–1060.

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Romanov, Y.I. Right-polarized neutral (anti)leptons in the solar neutrino flux. Bull. Russ. Acad. Sci. Phys. 79, 945–947 (2015). https://doi.org/10.3103/S1062873815040255

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  • DOI: https://doi.org/10.3103/S1062873815040255

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