Fermion masses and neutrino oscillations in SO(10) SUSY GUT with D(3) x U(1) family symmetry
Fermion masses and neutrino oscillations in SO(10) SUSY GUT with D(3) x U(1) family symmetry
复制标题
具有 D(3) x U(1) 族对称性的 SO(10) SUSY GUT 中的费米子质量和中微子振荡
DOI:
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发表时间:
1999
期刊:
影响因子:
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通讯作者:
S. Raby
中科院分区:
文献类型:
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作者:
R. Dermisek;S. Raby
Discrete non-Abelian gauge symmetries appear to be the most advantageous candidates for a family symmetry. We present a predictive $mathrm{SO}(10)$ SUSY GUT model with ${D}_{3}ifmmode imeselse exttimesfi{}U(1)$ family symmetry ${(D}_{3}$ is the dihedral group of order 6). The hierarchy in fermion masses is generated by the family symmetry breaking ${D}_{3}ifmmode imeselse exttimesfi{}U(1)ensuremath{
ightarrow}{Z}_{N}ensuremath{
ightarrow}mathrm{nothing}.$ This model fits the low energy data in the charged fermion sector quite well and naturally provides large angle ${ensuremath{
u}}_{ensuremath{mu}}ensuremath{-}{ensuremath{
u}}_{ensuremath{ au}}$ mixing describing atmospheric neutrino oscillation data and small angle ${ensuremath{
u}}_{e}ensuremath{-}{ensuremath{
u}}_{s}$ mixing consistent with the small mixing angle MSW solution to the solar neutrino data. In addition, the non-Abelian family symmetry ${D}_{3}$ is sufficient to suppress large flavor violations.