Abstract
The flavor composition of the solar beryllium neutrino was analyzed using schemes that include the new (heavy) neutrino (ν4) at a negligible angle of mixing with the light partners ν e , νμ, and ντ.
Similar content being viewed by others
References
Romanov, Yu.I., Slaboe vzaimodeistvie leptonov. Izbrannoe (Weak Interaction of Leptons. Selected Works), Moscow: MGUDT, 2009, Chapter V.
Ranucci, J., Nucl. Phys. B. Proc. Suppl., 2007, vol. 168, p. 111.
Arpesella, C., et al., (Borexino Collab.), Phys. Rev. Lett. B, 2008, vol. 658, p. 101.
Back, H.O., et al., (Borexino Collab.), Nucl. Instrum. Methods A, 2008, vol. 584, p. 98.
Back, H.O., et al., (Borexino Collab.), Nucl. Instrum. Methods A, 2008, vol. 585, p. 48.
Litvinovich, E.A., (Kollab. Boreksino), Yad. Fiz., 2009, vol. 72, no. 3, p. 558 [Phys. At. Nucl. (Engl. Transl.), 2009, vol. 72, no. 3, p. 522].
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © Yu.I. Romanov, 2010, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2010, Vol. 74, No. 6, pp. 861–863.
About this article
Cite this article
Romanov, Y.I. On the flavor composition of the solar 7Be neutrino. Bull. Russ. Acad. Sci. Phys. 74, 818–820 (2010). https://doi.org/10.3103/S1062873810060183
Published:
Issue Date:
DOI: https://doi.org/10.3103/S1062873810060183