2012
DOI: 10.1103/physrevd.86.117304
|View full text |Cite
|
Sign up to set email alerts
|

Nonzeroθ13signals nonmaximal atmospheric neutrino mixing

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
2

Citation Types

0
12
0

Year Published

2013
2013
2022
2022

Publication Types

Select...
5
1
1

Relationship

1
6

Authors

Journals

citations
Cited by 19 publications
(12 citation statements)
references
References 46 publications
0
12
0
Order By: Relevance
“…Subsequent to the first appearance [8] of Eq. (2), a further analysis in [9] found consistency of Eq. (2) with experiment, although at that time the RHS of Eq.…”
Section: Introductionmentioning
confidence: 74%
See 1 more Smart Citation
“…Subsequent to the first appearance [8] of Eq. (2), a further analysis in [9] found consistency of Eq. (2) with experiment, although at that time the RHS of Eq.…”
Section: Introductionmentioning
confidence: 74%
“…Among the 28 free parameters associated with the standard model of particle theory, the six mixing angles Θ ij and θ ij (1 ≤ i < j ≤ 3) associated respectively with the quarks [1,2] and the neutrinos [3,4] are the nearest to being calculable in a plausible theory. We have in mind the use of the binary tetrahedral group T ′ as a family symmetry following the discussion in [5][6][7][8][9].…”
Section: Introductionmentioning
confidence: 99%
“…In the latter approach, one needs now to correct significantly the leading-order predictions, by taking into account a number of sub-leading effects. After the measurement of a relatively large θ 13 , several flavour models have been proposed, that predict a non-zero value of θ 13 at leading order [8][9][10][11][12][13][14][15][16]. In fact, non-extreme, correlated values of the mixing angles are the generic prediction of discrete flavour symmetries [17,18].…”
Section: Jhep07(2013)146mentioning
confidence: 99%
“…In this vein, one popular parametrization was introduced in [39], which introduced deviations from TBM values using s, a, and r for the solar, atmospheric, and reactor mixing angles, respectively. Further work along this line, such as parameter scans in this space of deviations, include [40][41][42][43][44][45][46][47][48] and also [49][50][51][52], which used a similar approach but an equivalent set of parameters. One drawback of such approaches is that complete UV flavor models generally predict additional flavor violating effects, which are not captured in these low-energy deviation studies [53].…”
Section: Jhep02(2013)021mentioning
confidence: 99%