Status of the Standard Model of Particle Phenomenology.pdf

Status of the Standard Model of Particle Phenomenology.pdf

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Status of the Standard Model of Particle Phenomenology

a r X i v : h e p - p h / 0 3 1 0 2 1 7 v 1 1 7 O c t 2 0 0 3 Status of the Standard Model Paul H. Frampton University of North Carolina at Chapel Hill October 2003 1 Introduction The standard model is healthy is all respects except for the non-zero neutrino masses which require an extension of the minimal version. This talk was in three parts: (I) Rise and Fall of the Zee Model 1998-2001. (II) Classification of Two-Zero Textures. (III) FGY Model relating Cosmological B to Neutrino CP violation. For parts (I) and (II) references are provided. Part (III) is included in this write-up. 2 Rise and Fall of the Zee Model 1998-2001 This first part was based on: P.H. Frampton and S.L. Glashow, Phys. Lett. 461, 95 (1999). hep-ph/9906375. 3 Classification of Two-Zero Textures The second part was based on: P.H. Frampton, S.L. Glashow and D. Marfatia, Phys. Lett. B536, 79 (2002). hep-ph/0201008 4 FGY Model relating Cosmological B with Neu- trino CP Violation One of the most profound ideas is[1] that baryon number asymmetry arises in the early universe because of processes which violate CP symmetry and 1 that terrestrial experiments on CP violation could therefore inform us of the details of such cosmological baryogenesis. The early discussions of baryogenesis focused on the violation of baryon number and its possible relation to proton decay. In the light of present evidence for neutrino masses and oscillations it is more fruitful to associate the baryon number of the universe with violation of lepton number[2]. In the present Letter we shall show how, in one class of models, the sign of the baryon number of the universe correlates with the results of CP violation in neutrino oscillation experiments which will be performed in the forseeable future. Present data on atmospheric and solar neutrinos suggest that there are respective squared mass differences ?a ? 3×10?3eV 2 and ?s ? 5×10?5eV 2. The corresponding mixing angles θ1 and θ3 satisfy tan 2θ1 ? 1 and 0.6 ≤ sin22θ3 ≤ 0.

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