2002
DOI: 10.1016/s0550-3213(02)00570-9
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Structure of neutrino mass matrix and CP-violation

Abstract: We reconstruct the neutrino mass matrix in the flavor basis, using all available experimental data from neutrino oscillations. Majorana nature of neutrinos, normal mass hierarchy (ordering) and validity of the LMA MSW solution of the solar neutrino problem are assumed. We study dependences of the mass matrix elements, m αβ , on the CP violating Dirac, δ, and Majorana, ρ, σ, phases, for different values of the mixing angle θ 13 and of the absolute mass scale, m 1 . The contours of constant mass in the ρ − σ pla… Show more

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Cited by 74 publications
(44 citation statements)
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“…Being a symmetric matrix, m ν contains six independent and complex entries, corresponding to nine physical parameters. Several analyzes [3,4,5] have been performed in order to study the form of the neutrino mass matrix as allowed by current data. Reconstructing m ν is possible since for Majorana neutrinos -in contrast to the quark sector -the mass matrix is in general symmetric.…”
Section: Introductionmentioning
confidence: 99%
“…Being a symmetric matrix, m ν contains six independent and complex entries, corresponding to nine physical parameters. Several analyzes [3,4,5] have been performed in order to study the form of the neutrino mass matrix as allowed by current data. Reconstructing m ν is possible since for Majorana neutrinos -in contrast to the quark sector -the mass matrix is in general symmetric.…”
Section: Introductionmentioning
confidence: 99%
“…With the present accuracy of measurements of the parameters, a sharp difference between dominant and subdominant elements may not exist and some moderate hierarchy of elements with the unique expansion parameter 0.6 -0.7 is realized [39].…”
Section: Extreme Casesmentioning
confidence: 93%
“…Results of reconstruction show [39] that a large variety of different structures of mass matrices is possible, depending strongly on the unknown m 1 , type of mass hierarchy and Majorana phases. The dependence on sin θ 13 and δ is relatively weak.…”
Section: B Reconstructing Neutrino Mass Matrixmentioning
confidence: 99%
“…(3.2), (3.3) and (3.5)) can be rewritten as functions of the low-energy observables using the expressions of m αβ in terms of the masses and mixing of light neutrinos [21,22,23]. In the limit θ 13 = 0 and θ 23 = π/4, we find from Eq.…”
Section: The Generic Casementioning
confidence: 99%
“…Using this phenomenological information one can, to a large extent, reconstruct the mass matrix m, just by inserting the data (2.3) -(2.4) into Eq. (2.1) [21,22,23]. A significant freedom still exists due to the unknown absolute mass scale |m 1 | and CP-violating phases ρ, σ.…”
Section: Low Energy Data and Structure Of Light Neutrino Mass Matrixmentioning
confidence: 99%