Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1992-05-09
Phys.Rev. D46 (1992) 3034-3039
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, 2 figures (not included)
Scientific paper
10.1103/PhysRevD.46.3034
The oscillations of pseudo-Dirac neutrinos in matter are discussed and applied to the solar neutrino problem. Several scenarios such as both $\nu_e$ and $\nu_{\mu}$ being pseudo-Dirac and only $\nu_e$ or $\nu_{\mu}$ being pseudo-Dirac are examined. It is shown that the allowed region in the mass-mixing angle parameter space obtained by comparing the solar neutrino data with the calculations based on the standard solar model and the MSW effect is not unique. The results depend on the nature of neutrinos; for example, if both $\nu_e$ and $\nu_{\mu}$ are pseudo-Dirac, the allowed region determined by the current solar neutrino data does not overlap with that obtained in the usual case of pure Dirac or Majorana neutrinos.
Giunti Carlo
Kim Chung Wook
Lee U. W.
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