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An alternative: two-mixing texture for three neutrinos or three-mixing texture for four neutrinos

2000/08/16 by Wojciech Krolikowski
Physics and Astronomy · #hep-ph

paper · pdf

published as Acta Phys.Polon. B32 (2001) 75-84 · 1+8 pages

arxiv created 2000/08/16 · arxiv updated 2009/11/30

Abstract

The alternative formulated in the title has a chance to be settled, when the existence of the LSND effect is experimentally excluded or confirmed. The first option, much discussed in literature, works in the case of three active neutrinos νe, νμ, ντ, when among their massive states ν1, ν2, ν3 there is no direct mixing between ν1 and ν3, and the mass hierarchy m21 < ∼ m22 ≪ m23 holds. This option is consistent with the observed deficits of solar νe's and atmospheric νμ's, if Δm221 ↔ Δm2\rm sol and Δm232 ↔ Δm2\rm atm. On the other hand, the second option is an extension of the idea of the former to the case of four neutrinos νs, νe, νμ, ντ (including one sterile neutrino νs), when among their massive states ν0, ν1, ν2, ν3 there are no direct mixings between ν0 and nu2, ν0 and ν3, ν1 and ν3, and the mass hierarchy m20 < ∼ m21 ≪ m22 < ∼ m23 is now valid. Such an option, belonging to a class of textures widely discussed in literature, may be consistent with the observed deficits of solar νe's and atmospheric νμ's as well as with the LSND appearance of νe's in the beam of accelerator νμ's, if now Δm210 ↔ Δm2\rm sol, Δm232 ↔ Δm2\rm atm and Δm221 ↔ Δm2\rm LSND.

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