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Flavor Mixing Neutri no Masses

This article explores the flavor mixing in particle physics, focusing on the CKM matrix for quarks and the neutrino mixing matrix. It discusses the observed quark masses, Cabibbo angle, unitarity triangle, and the connection to neutrino oscillations. The experiments of Fritzsch, Pontecorvo, Kamiokande, SNO, and the Nobel Prize-winning discoveries are also discussed.

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Flavor Mixing Neutri no Masses

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  1. Flavor Mixing NeutrinoMasses and H. Fritzsch

  2. c u t d s b flavor mixing

  3. CKM - matrix

  4. Experiments

  5. :H. Fritzsch – Z. Xing

  6. experiments

  7. flavor mixing angles - fermion masses

  8. - - III 2 families flavor mixing II I

  9. mass matrices texture 0 H. Fritzsch - S. Weinberg / 1978

  10. SO(10)

  11. mixing angles <=> masses

  12. Observedquarkmasses

  13. Cabibbo angle

  14. Cabibbo angle

  15. - 3 families III flavor mixing II I

  16. - texture zeros

  17. m: GeV

  18. - unitarity triangle

  19. Cabibbo angle unitarity triangle (rectangular)

  20. mixing of leptons

  21. Bruno Pontecorvo 1913 - 1993

  22. neutrino mixing

  23. B. Pontecorvo Phys. JETP 6, 429 (1957) H. Fritzsch - P. Minkowski Physics Letters 62B, 76 (1975)

  24. Neutrino oscillations

  25. Fritzsch – Minkowski (1975)

  26. Kamioka

  27. Atmospheric neutrinos

  28. neutrino oscillations Ewigkeit ist lang, speziell gegen dem Ende zu. W.A.

  29. YoJI Totsuka Ewigkeit ist lang, speziell gegen dem Ende zu. W.A.

  30. Nobel prize 2015 Kajita Ewigkeit ist lang, speziell gegen dem Ende zu. W.A. TakaakiKajita

  31. 2001 => Canada Sudbury Neutrino Obervatory SNO

  32. S N O Solar neutrinos charged current neutral current

  33. Arthur McDonald Nobel Prize 2015

  34. flavor mixing leptons

  35. neutrino mixing matrix (==> CKM Matrix)

  36. V = U P Fritzsch - Xing

  37. n Kamiokande - SNO

  38. - texture zeros

  39. observation

  40. ==> neutrino masses

  41. neutrinomasses ( eV )

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