Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2001-04-23
Phys.Rev. D64 (2001) 077301
Physics
High Energy Physics
High Energy Physics - Phenomenology
Latex file, 10 pages, 1 figure, explanations and references added, typos corrected, to be published in Phys.Rev.D
Scientific paper
10.1103/PhysRevD.64.077301
The eigenvalues and mixing angles in the Zee model are investigated parameter-independently. When we require |\Delta m^2_{12}/\Delta m^2_{23}| \ll 1 in order to understand the solar and atmospheric data simultaneously, the only solution is one which gives bi-maximal mixing. It is pointed out that the observed values \sin^2 2\theta_{solar} \simeq 0.66 in the MSW LMA solution cannot be explained within the framework of the Zee model, because we derive a severe constraint on the value of \sin^2 2 \theta_{solar}, \sin^2 2 \theta_{solar} \geq 1 -(1/16)(\Delta m^2_{solar}/\Delta m^2_{atm})^2.
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