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Neutrino oscillations in the dualized standard model

José Bordes*

Chan Hong-Mo†

Jakov Pfaudler‡

Tsou Sheung Tsun§

  • Deptartament Fisica Teorica, Universitat de Valencia, calle Dr. Moliner 50, E-46100 Burjassot (Valencia), Spain

  • Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, OX11 0QX, United Kingdom

  • Department of Physics, Theoretical Physics, University of Oxford, 1 Keble Road, Oxford, OX1 3NP, United Kingdom

  • Mathematical Institute, University of Oxford, 24-29 St. Giles’, Oxford, OX1 3LB, United Kingdom

  • *E-mail address: bordes@evalvx.ific.uv.es
  • †E-mail address: chanhm@v2.rl.ac.uk
  • ‡E-mail address: jakov@thphys.ox.ac.uk
  • §E-mail address: tsou@maths.ox.ac.uk
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Phys. Rev. D 58, 053003 – Published 17 July, 1998

DOI: https://doi.org/10.1103/PhysRevD.58.053003

Abstract

A method developed from the dualized standard model for calculating the quark CKM matrix and masses is applied to the parallel problem in neutrino oscillations. Taking the parameters determined from quarks and the masses of two neutrinos: m32∼10−2–10−3 eV2 suggested by atmospheric neutrino data and m22∼10−10 eV2 suggested by the long-wavelength oscillation solution of the solar neutrino problem, one obtains from a parameter-free calculation all the mixing angles in reasonable agreement with existing experiments. However, the scheme is found not to accommodate comfortably the mass values m22∼10−5 eV2 suggested by the MSW solution for solar neutrinos.

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References (24)

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Phys. Rev. D 58, 053003– Published 17 July, 1998
  • Received 25 February 1998

© 1998 American Physical Society

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