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Monday, July 13, 2020 | History

2 edition of Tri-maximal vs. bi-maximal neutrino mixing found in the catalog.

Tri-maximal vs. bi-maximal neutrino mixing

W. G. Scott

Tri-maximal vs. bi-maximal neutrino mixing

by W. G. Scott

  • 177 Want to read
  • 27 Currently reading

Published by Rutherford Appleton Laboratory in Chilton .
Written in English


Edition Notes

StatementW.G. Scott.
SeriesRutherford Appleton Laboratory Technical Report -- RAL-TR-1999-066
ContributionsRutherford Appleton Laboratory., Council For The Central Laboratory of The Research Councils.
ID Numbers
Open LibraryOL21872266M


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Tri-maximal vs. bi-maximal neutrino mixing by W. G. Scott Download PDF EPUB FB2

Tri-maximal vs. bi-maximal neutrino mixing Article in Nuclear Physics B - Proceedings Supplements 85(1) May with 3 Reads How we measure 'reads'.

Tri-Maximal vs. Bi-Maximal Neutrino Mixing W. Scott Rutherford Appleton Laboratory, Chilton, Didcot, UK. It is argued that data from atmospheric and solar neutrino experiments point strongly to tri-maximal or bi-maximal lepton mixing.

While (‘optimised’) bi-maximal mixing gives an excellent a posteriori fit to the data. It is argued that data from atmospheric and solar neutrino experiments point strongly to tri-maximal or bi-maximal lepton mixing. While (‘optimised’) bi-maximal mixing gives an excellent a posteriori fit to the data, tri-maximal mixing is an a priori hypothesis, which is not excluded, taking account of terrestrial matter by: 2.

bi-maximal [5] and tri-maximal [3] structures in a single mi xing matrix of (). But there exists another complication due to the hypothetical mechanism for generating neutrino masses.

The observed large mixing angles in the lepton sector may be the first signal for the presence of a non-Abelian family symmetry. However, to obtain th Cited by: () Tri-maximal vs. bi-maximal neutrino mixing. Nuclear Physics B - Proceedings Supplements() Classroom Note:Centrosymmetric by: In this paper a special class of matrices W in $\mathcal{C}^{n \times n} $ that are a generalization of reflexive and antireflexive matrices are introduced, their fundamental properties are develop Cited by: In this paper a special class of matrices W in $\mathcal{C}^{n \times n} $ that are a generalization of reflexive and antireflexive matrices are introduced, their fundamental properties are develop.

Another possibility is to assume a bi-maximal form for the neutrino mass and a tri-maximal form for the charged lepton mass as done in Ref.

[3]. Certainly, the latter choice is very appealing in the simplicity of explaining both the bi-maximal [5] and tri-maximal [3] Read: Boyar Sky - Free download as PDF File .pdf), Text File .txt) or read online for free. Boyar. Full text of "Particle physics in the new millennium: proceedings of the 8th Adriatic meeting" See other formats.

Within this standard parameterization, the 6 + 3 neutrino parameters are the 3 neutrino mass eigenvalues, m1, m2, m3, the 3 mixing angles θij and the 3 CP -violating phases φ, α and β. φ is the analogous of the CKM phase, and affects the flavour content of the neutrino mass eigenstates. α and β are called “Majorana phases” and.