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Constraints on flavor neutrino masses and sin{sup 2}2{theta}{sub 12}>>sin{sup 2}{theta}{sub 13} in neutrino oscillations

Journal Article · · Physical Review. D, Particles Fields
; ;  [1]
  1. Department of Physics, Tokai University, 1117 Kitakaname, Hiratsuka, Kanagawa 259-1291 (Japan)
To realize the condition of sin{sup 2}2{theta}{sub 12}>>sin{sup 2}{theta}{sub 13}, we find constraints on flavor neutrino masses M{sub ij} (ij=e,{mu},{tau}): (C1) c{sub 23}{sup 2}M{sub {mu}}{sub {mu}}+s{sub 23}{sup 2}M{sub {tau}}{sub {tau}}{approx_equal}2s{sub 23}c{sub 23}M{sub {mu}}{sub {tau}}+M{sub ee} and/or (C2) vertical bar c{sub 23}M{sub e{mu}}-s{sub 23}M{sub e{tau}} vertical bar >> vertical bar s{sub 23}M{sub e{mu}}+c{sub 23}M{sub e{tau}} vertical bar, where c{sub 23}=cos{theta}{sub 23} (s{sub 23}=sin{theta}{sub 23}) and {theta}{sub 12}, {theta}{sub 13}, and {theta}{sub 23} are the mixing angles for three flavor neutrinos. The applicability of (C1) and (C2) is examined in models with one massless neutrino and two massive neutrinos suggested by det(M)=0, where M is a mass matrix constructed from M{sub ij} (i,j=e,{mu},{tau}). To make definite predictions on neutrino masses and mixings, especially on sin{theta}{sub 13}, that enable us to trace (C1) and (C2), M is assumed to possess texture zeros or to be constrained by textures with M{sub {mu}}{sub {mu}}=M{sub {tau}}{sub {tau}} or M{sub e{tau}}={+-}M{sub e{mu}}, which turn out to ensure the emergence of the maximal atmospheric neutrino mixing at sin{theta}{sub 13}{yields}0. It is found that (C1) is used by textures such as M{sub e{mu}}=0 or M{sub e{tau}}=0, while (C2) is used by textures such as M{sub e{tau}}={+-}M{sub e{mu}}.
OSTI ID:
20709010
Journal Information:
Physical Review. D, Particles Fields, Journal Name: Physical Review. D, Particles Fields Journal Issue: 7 Vol. 71; ISSN PRVDAQ; ISSN 0556-2821
Country of Publication:
United States
Language:
English

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