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Neutrino oscillations in the dualized standard model

Feb, 1998
16 pages
Published in:
  • Phys.Rev.D 58 (1998) 053003
e-Print:
DOI:
Report number:
  • RAL-TR-98-021
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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∼10−2−10−3eV2m_3^2 \sim 10^{-2} - 10^{-3} eV^2 suggested by atmospheric neutrino data, and m22∼10−10eV2m_2^2 \sim 10^{-10} eV^2 suggested by the long wave-length oscillation (LWO) solution of the solar neutrino problem, one obtains from a parameter-free calculation all the mixing angles in reasonable agreement with existing experiment. However, the scheme is found not to accommodate comfortably the mass values m22∼10−5eV2m_2^2 \sim 10^{-5} eV^2 suggested by the MSW solution for solar neutrinos.
  • neutrino: oscillation
  • gauge field theory: SU(3) x SU(2) x U(1)
  • duality
  • neutrino: mass
  • neutrino: cosmic radiation
  • neutrino: solar
  • neutrino: mixing angle
  • CKM matrix: leptonic
  • numerical calculations
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