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Quark-Lepton complementarityRecent neutrino experiments confirm that
the Pontecorvo-Maki-Nakagawa-Sakata
(PMNS) lepton mixing matrix UPMNS contains large mixing angles.
For example the atmospheric mixing UNIQ3ca1dfa4675b419e-math-00000002-QINU
is compatible with UNIQ3ca1dfa4675b419e-math-00000003-QINU,
and the solar mixing UNIQ3ca1dfa4675b419e-math-00000004-QINU is
UNIQ3ca1dfa4675b419e-math-00000005-QINU.
These results should be compared with the third lepton mixing angle
Additional recommended knowledgeThe disparity that nature indicates between quark and lepton mixing angles has been viewed in terms of a 'quark-lepton complementarity' (QLC) which can be expressed in the relations Possible consequences
of QLC have been investigated in the literature
and in particular a simple correspondence between the
UPMNS and UCKM
matrices has been proposed
and analyzed in terms of a
correlation matrix.
The correlation matrix VM
is simply defined as the product
of the CKM and
PMNS matrices,
Furthermore in some Grand Unification Theories (GUTs) the direct QLC correlation between the CKM and the PMNS mixing matrix can be obtained. In this class of models, the VM matrix is determined by the heavy Majorana neutrino mass matrix. Despite the naive relations between the PMNS and CKM angles, a detailed analysis shows that the correlation matrix is phenomenologically compatible with a tribimaximal pattern, and only marginally with a bimaximal pattern. It is possible to include bimaximal forms of the correlation matrix VM in models with renormalization effects that are relevant, however, only in particular cases with large tanβ( > 40) and with quasi degenerate neutrino masses. References
"Quark-lepton complementarity, neutrino and standard model data predict |
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Quark-Lepton_complementarity". A list of authors is available in Wikipedia. |