TY - JOUR
T1 - Neutrino mixing and see-saw mechanism
AU - Jezabek, M.
AU - Sumino, Y.
N1 - Funding Information:
This work is partly supported by KBN grant 2P03B08414, by BMBF grant POL-239-96 and by the Alexander von Humboldt Foundation.
PY - 1998/11/19
Y1 - 1998/11/19
N2 - Models of neutrino masses are discussed capable of explaining in a natural way the maximal mixing between νμ and ντ observed by the Super-Kamiokande Collaboration. For three generations of leptons two classes of such models are found implying: a) Δm223 ≪ Δm212 ≈ Δm213 and a small mixing between νe and the other two neutrinos, b) Δm212 ≪ Δm213 = Δm223 and a nearly maximal mixing for solar neutrino oscillations in vacuum.
AB - Models of neutrino masses are discussed capable of explaining in a natural way the maximal mixing between νμ and ντ observed by the Super-Kamiokande Collaboration. For three generations of leptons two classes of such models are found implying: a) Δm223 ≪ Δm212 ≈ Δm213 and a small mixing between νe and the other two neutrinos, b) Δm212 ≪ Δm213 = Δm223 and a nearly maximal mixing for solar neutrino oscillations in vacuum.
UR - http://www.scopus.com/inward/record.url?scp=0000000181&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0000000181&partnerID=8YFLogxK
U2 - 10.1016/S0370-2693(98)01113-7
DO - 10.1016/S0370-2693(98)01113-7
M3 - Article
AN - SCOPUS:0000000181
SN - 0370-2693
VL - 440
SP - 327
EP - 331
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
IS - 3-4
ER -