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Brooks Thomas (University of Michigan, MCTP)

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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Brooks Thomas (University of Michigan, MCTP)

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  1. Dirac Leptogenesis and Neutrino Phenomenology The CMB as seen by WMAP Brooks Thomas (University of Michigan, MCTP)

  2. Superpotential and Fields Effective Dirac Mass

  3. Two Distinct Lepton Numbers SU(2)£ U(1) Left-right equilibration (suppressed) Lagg LR F

  4. 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

  5. yeff y’ L-R Equilibration Process Constraints: Delayed Equilibration

  6. Constraints: Gravitino Problem BBN Constraints PeV Window Most Favorable Region Gluino Problem

  7. Constraints: Neutrino Physics Atmospheric Solar (LMA) sin31

  8. The Normal Spectrum Neutrinos In Dirac Leptogenesis

  9. CHDL: a Theory-Motivated Model

  10. CHDL and the Neutrino Spectrum a3 and b3 for =10-1 a3 and b3 in CHDL

  11. Solving the Boltzmann Equations Dominant Weak Coupling Solution Strong Coupling Solution

  12. 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

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