2005
DOI: 10.1103/physrevd.71.097301
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Unified parametrization of quark and lepton mixing matrices

Abstract: We present a unified parametrization of quark and lepton mixing matrices. By using some simple relations between the mixing angles of quarks and leptons, i.e., the quark-lepton complementarity, we parametrize the lepton mixing matrix with the Wolfenstein parameters λ and A of the quark mixing matrix. It is shown that the Wolfenstein parameter λ can measure both the deviation of the quark mixing matrix from the unit matrix, and the deviation of the lepton mixing matrix from the exactly bimaximal mixing pattern.… Show more

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Cited by 58 publications
(51 citation statements)
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“…We will omit the Majorana phases for simplicity; it was shown that they interplay with the CP phase in some entries of the exponential matrix and just produce more complex terms (see [35]). Let us consider first of all only the real rotational part and compare the rotational matrix (18) with the TBM form of the mixing matrix [20,28]. With the help of (19), (20), (21), (22), we obtain the following values for the parameters of the exponential parameterization (18), corresponding to the TBM parameterization: • .…”
Section: Real Rotation Matrix and The Current Experimental Datamentioning
confidence: 99%
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“…We will omit the Majorana phases for simplicity; it was shown that they interplay with the CP phase in some entries of the exponential matrix and just produce more complex terms (see [35]). Let us consider first of all only the real rotational part and compare the rotational matrix (18) with the TBM form of the mixing matrix [20,28]. With the help of (19), (20), (21), (22), we obtain the following values for the parameters of the exponential parameterization (18), corresponding to the TBM parameterization: • .…”
Section: Real Rotation Matrix and The Current Experimental Datamentioning
confidence: 99%
“…Let us consider first of all only the real rotational part and compare the rotational matrix (18) with the TBM form of the mixing matrix [20,28]. With the help of (19), (20), (21), (22), we obtain the following values for the parameters of the exponential parameterization (18), corresponding to the TBM parameterization: • . (33) Now, from the data set, reported in [14,28], we obtain for neutrinos To avoid the uncertainty, originating from largely undetermined CP-violating phase, we calculated the fit with the experimentally determined values of the entries of the PMNS matrix, which contain only the mixing angles θ i, j and do not depend on the CP violation, described by δ.…”
Section: Real Rotation Matrix and The Current Experimental Datamentioning
confidence: 99%
See 2 more Smart Citations
“…[3] are given in Table I Initially neutrino oscillation experiments indicated the atmospheric mixing angle, θ 23 is maximal i.e., θ 23 = π/4 and reactor mixing angle θ 13 is vanishingly small and motivated by such anticipation many models for neutrino mixing were proposed such as Bimaximal mixing (BM) [6][7][8][9][10][11], Tri-bimaximal mixing (TBM) [12][13][14][15][16][17][18][19][20], Golden ratio type-A (GRA), type-B (GRB) [21,22] and Hexagonal mixing (HG), etc. All such models are based on some discrete symmetries such as A 4 , S 4 [23,24] etc and can be represented as…”
Section: Introductionmentioning
confidence: 99%