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'''Trimaximal mixing'''<ref name="HPS1999">
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{{cite journal
| author=P.F. Harrison, D. H. Perkins and W. G. Scott
| year=1999
| title=A Redetermination of the Neutrino Mass-Squared Difference in Tri-Maximal Mixing with Terrestrial Matter Effects
| journal=[[Physics Letters B]]
| volume=458 |issue=1 | pages=79
| arxiv=hep-ph/9904297
| bibcode=1999PhLB..458...79H
| doi=10.1016/S0370-2693(99)00438-4
}}</ref> (also known as threefold maximal mixing<ref name="HPS1995">
{{cite journal
| author=P.F. Harrison, D. H. Perkins and W. G. Scott
| year=1995
| title=Threefold Maximal Lepton Mixing and the Solar and Atmospheric Neutrino Deficits
| url=http://www-lib.kek.jp/cgi-bin/img_index?9503190
| journal=[[Physics Letters B]]
| volume=349 |issue=1–2 | pages=137
| bibcode=1995PhLB..349..137H
| doi=10.1016/0370-2693(95)00213-5
}}</ref>) refers to the highly symmetric, maximally CP-violating, <math>3 \times 3</math> [[fermion]] mixing configuration, characterised by a [[unitary matrix]] (<math>U</math>) having all its elements equal in modulus
(<math> |U_{ai}|=1/\sqrt{3}</math>, <math>a,i=1,2,3</math>) as may be written, e.g.:
 
:<math>
U=
\begin{bmatrix}
\frac{1}{\sqrt{3}} & \frac{1}{\sqrt{3}} & \frac{1}{\sqrt{3}} \\
\frac{\omega}{\sqrt{3}} & \frac{1}{\sqrt{3}} & \frac{\bar{\omega}}{\sqrt{3}} \\
\frac{\bar{\omega}}{\sqrt{3}} & \frac{1}{\sqrt{3}} & \frac{\omega}{\sqrt{3}}
\end{bmatrix}
\Rightarrow (|U_{i\alpha}|^2)=
\begin{bmatrix}
\frac{1}{3} & \frac{1}{3} & \frac{1}{3} \\
\frac{1}{3} & \frac{1}{3} & \frac{1}{3} \\
\frac{1}{3} & \frac{1}{3} & \frac{1}{3}
\end{bmatrix}
</math>
 
where <math>\omega=\exp(i2\pi/3)</math> and <math>\bar{\omega}=\exp(-i2\pi/3)</math>
are the complex [[cube roots]] of unity. In the standard PDG<ref name="PDG">
{{cite journal
| author=W.M. Yao ''et al.''
| year=2006
| title=Review of Particle Physics: Neutrino mass, mixing, and flavor change
| url=http://pdg.lbl.gov/2006/reviews/numixrpp.pdf
| journal=[[Journal of Physics G]]
| volume=33 |page=1
|arxiv = astro-ph/0601168 |bibcode = 2006JPhG...33....1Y |doi = 10.1088/0954-3899/33/1/001 }}</ref> convention, trimaximal mixing corresponds to: <math>\theta_{12}=\theta_{23}=\pi/4</math>, <math>\theta_{13}=\sin^{-1}(1/\sqrt{3})</math> and <math>\delta=\pi/2</math>. The Jarlskog <math>CP</math>-violating parameter <math>J</math><ref name="JCP">
{{cite journal
| author=C. Jarlskog
| year=1985
| title=Commutator of the Quark Mass Matrices in the Standard Electroweak Model and a Measure of Maximal <math>CP</math> Non-Conservation
| journal=[[Physical Review Letters]]
| volume=55 | issue=10 | pages=1039
| bibcode=1985PhRvL..55.1039J
| doi=10.1103/PhysRevLett.55.1039
| pmid=10031712
}}</ref> takes its extremal value <math>|J|=1/(6\sqrt{3})</math>.
 
Originally proposed as a candidate [[neutrino oscillation|lepton mixing]] matrix,<ref name="WOLF78">
{{cite journal
| author=L. Wolfenstein
| year=1978
| title=Oscillations Among Three Neutrino Types and CP Violation
| journal=[[Physical Review D]]
| volume=18 |issue=3 | pages=958
| bibcode=1978PhRvD..18..958W
| doi=10.1103/PhysRevD.18.958
}}</ref><ref name="CAB78">
{{cite journal
| author=N. Cabibbo
| year=1978
| title=Time Reversal Violation in Neutrino Oscillation
| journal=[[Physics Letters B]]
| volume=32 |issue=3 | pages=333
| bibcode=1978PhLB...72..333C
| doi=10.1016/0370-2693(78)90132-6
}}</ref> and actively studied<ref name="HPS1999"/><ref name="HPS1995"/><ref name="GIUNTI1995">
{{cite journal
| author=C. Giunti, C. W. Kim and J. D. Kim,
| year=1995
| title=Atmospheric Neutrino Problem in Maximally Mixed Three Generations of Neutrinos
| journal=[[Physics Letters B]]
| volume=352 |issue=3–4 | pages=357
| arxiv=hep-ph/9411219
| bibcode=1995PhLB..352..357G
| doi=10.1016/0370-2693(95)00424-J
}}</ref><ref name="HPS1997">
{{cite journal
| author=P.F. Harrison, D. H. Perkins and W. G. Scott
| year=1997
| title=Further Evidence for Threefold Maximal Lepton Mixing and a Hierarchical Spectrum of Neutrino Mass-Squared Differences
| journal=[[Physics Letters B]]
| volume=396 |issue=1–4 | pages=186
| arxiv=hep-ph/9702243
| bibcode=1997PhLB..396..186H
| doi=10.1016/S0370-2693(97)00105-6
}}</ref> as such (and even as a candidate quark mixing matrix<ref name="HS1994">
{{cite journal
| author=P.F. Harrison and W. G. Scott
| year=1994
| title=Generation Permutation Symmetry and the Quark Mixing Matrix
| journal=[[Physics Letters B]]
| volume=333 |issue=3–4 | pages=471
| arxiv=hep-ph/9406351
| bibcode=1994PhLB..333..471H
| doi=10.1016/0370-2693(94)90170-8
}}</ref>), trimaximal mixing is now definitively ruled-out as a phenomenologically viable lepton mixing scheme by [[neutrino oscillation]] experiments, especially the [[CHOOZ]] reactor experiment,<ref name="CHOOZ">
{{cite journal
| author=M. Apollonio et al.
| year=2003
| title=Search for Neutrino Oscillations on a Long Baseline at the CHOOZ Nuclear Power Station
| journal=[[European Physical Journal C]]
| volume=27 |issue=3 | pages=331
| arxiv=hep-ex/0301017
| bibcode=2003EPJC...27..331A
| doi=10.1140/epjc/s2002-01127-9
}}</ref> in favour of the no longer tenable (related) [[tribimaximal mixing]]<ref name="HPS2002">
{{cite journal
| author=P.F. Harrison, D. H. Perkins and W. G. Scott
| year=2002
| title=Tri-Bimaximal Mixing and the Neutrino Oscillation Data
| journal=[[Physics Letters B]]
| volume=530 |issue=1–4 | pages=167
| arxiv=hep-ph/0202074
| bibcode=2002PhLB..530..167H
| doi=10.1016/S0370-2693(02)01336-9
}}</ref> scheme.
 
==References==
{{reflist|2}}
 
[[Category:Leptons]]
[[Category:Standard Model]]
[[Category:Particle physics]]

Latest revision as of 04:01, 14 May 2014

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