An expansion for neutrino phenomenology

被引:9
|
作者
Grinstein, Benjamin [1 ]
Trott, Michael [2 ]
机构
[1] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[2] CERN, Div Theory, Dept Phys, CH-1211 Geneva 23, Switzerland
来源
关键词
Neutrino Physics; Solar and Atmospheric Neutrinos; SOLAR NEUTRINOS; QUARK MASSES; DOMINANCE; ANGLES; MODELS;
D O I
10.1007/JHEP09(2012)005
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We develop a formalism for constructing the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) matrix and neutrino masses using an expansion that originates when a sequence of heavy right handed neutrinos are integrated out, assuming a seesaw mechanism for the origin of neutrino masses. The expansion establishes relationships between the structure of the PMNS matrix and the mass differences of neutrinos, and allows symmetry implications for measured deviations from tri-bimaximal form to be studied systematically. Our approach does not depend on choosing the rotation between the weak and mass eigen-states of the charged lepton fields to be diagonal. We comment on using this expansion to examine the symmetry implications of the recent results from the Daya-Bay collaboration reporting the discovery of a non zero value for theta(13), indicating a deviation from tri-bimaximal form, with a significance of 5.2 sigma.
引用
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页数:16
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