2013
DOI: 10.1103/physrevd.88.093007
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Relating neutrino masses and mixings by discrete symmetries

Abstract: Lepton mixing can originate from the breaking of a flavor symmetry in different ways in the neutrino and the charged lepton sector. We propose an extension of this framework which allows to connect the mixing parameters with masses, and more precisely, with certain types of degeneracy of the neutrino mass spectrum. We obtain relations between the mixing parameters for the cases of partial degeneracy, m 1 = m 2 , and complete degeneracy, m 1 = m 2 = m 3 . These relations determine also the Majorana phases. It i… Show more

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Cited by 30 publications
(39 citation statements)
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“…In this case with the solution tag C 4 , the seventh root of unity, γ = e 2πi/7 , occurs in the eigenvalues and the mixing matrix reads 18) where the r i are the roots of the equation…”
Section: Jhep09(2014)033mentioning
confidence: 99%
See 1 more Smart Citation
“…In this case with the solution tag C 4 , the seventh root of unity, γ = e 2πi/7 , occurs in the eigenvalues and the mixing matrix reads 18) where the r i are the roots of the equation…”
Section: Jhep09(2014)033mentioning
confidence: 99%
“…In recent years, assuming neutrinos are Majorana particles, much effort has gone into the discussion of the lepton mixing matrices U from residual symmetries. Though a lot of results have been achieved [6][7][8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23][24], the present status has not been reached in a systematic way. 1 Thus it is by no means clear if the cases existing in the literature encompass all relevant mixing matrices.…”
Section: Introductionmentioning
confidence: 99%
“…(1.2) and DSG of SU(3). This was studied for the finite von-Dyck groups in [21] and for all DSG of SU(3) having three dimensional IR in [22]. Here, the third state is not implied to be massless.…”
Section: Jhep11(2015)186mentioning
confidence: 99%
“…In the semi-direct models a continuous parameter is introduced, derived from the freedom to rotate in the degenerate subspace of the neutrino residual symmetry, allowing the prediction of * jessica.turner@durham.ac.uk a non-zero θ 13 . There are several attractive features of implementing such an approach: firstly a UV-complete theory is not necessary in order to predict leptonic observables [16][17][18][19][20][21][22]. Secondly, correlations between the observables can be derived and provide specific signatures which allow the comparison of a range of models to experimental data [18][19][20][21][22][23][24][25].…”
Section: Introductionmentioning
confidence: 99%