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Dirac Leptogenesis and Neutrino Phenomenology. The CMB as seen by WMAP. Brooks Thomas (University of Michigan, MCTP). Superpotential and Fields. Effective Dirac Mass. Two Distinct Lepton Numbers. SU(2) £ U(1). Left-right equilibration (suppressed). L agg. L R. F . B. B. B. L. L.
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Dirac Leptogenesis and Neutrino Phenomenology The CMB as seen by WMAP Brooks Thomas (University of Michigan, MCTP)
Superpotential and Fields Effective Dirac Mass
Two Distinct Lepton Numbers SU(2)£ U(1) Left-right equilibration (suppressed) Lagg LR F
B B B L L L A Game of Time Scales 1 2 3 Positive B Positive L (B-L)=Const. Lagg Lagg LR Lagg LR LR Initial Decays Sphaleron Era Equilibration Era
yeff y’ L-R Equilibration Process Constraints: Delayed Equilibration
Constraints: Gravitino Problem BBN Constraints PeV Window Most Favorable Region Gluino Problem
Constraints: Neutrino Physics Atmospheric Solar (LMA) sin31
The Normal Spectrum Neutrinos In Dirac Leptogenesis
CHDL and the Neutrino Spectrum a3 and b3 for =10-1 a3 and b3 in CHDL
Solving the Boltzmann Equations Dominant Weak Coupling Solution Strong Coupling Solution
E X C L U D E D E X C L U D E D a3=95.0 a3=4.5 The Final Result: CHDL Works