Leptogenesis, mu - tau symmetry and
Feb, 200516 pages
Published in:
- Phys.Lett.B 615 (2005) 231-239
e-Print:
- hep-ph/0502026 [hep-ph]
Report number:
- UMD-PP-05-040
View in:
Citations per year
Abstract: (Elsevier)
We show that in theories where neutrino masses arise from type I see-saw formula with three right-handed neutrinos and where large atmospheric mixing angle owes its origin to an approximate leptonic μ – τ interchange symmetry, the primordial lepton asymmetry of the Universe, εl can be expressed in a simple form in terms of low energy neutrino oscillation parameters as εl=(aΔm⊙2+bΔmA2θ132) , where a and b are parameters characterizing high scale physics and are each of order ⩽10−2 eV−2 . We also find that for the case of two right-handed neutrinos, εl∝θ132 as a result of which, the observed value of baryon to photon ratio implies a lower limit on θ13 . For specific choices of the CP phase δ we find θ13 is predicted to be between 0.10–0.15.- lepton: production
- lepton: asymmetry
- neutrino: right-handed
- neutrino: mass
- neutrino: mixing angle
- seesaw model
- neutrino: oscillation
- CP: violation
- muon tau: symmetry
- numerical calculations
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- [5]
- [5]
- [6]
- [7]
- [8]
- [9]
- [9]
- [9]
- [10]
- [11]
- [11]
- [11]
- [11]
- [12]
- [13]
- [14]
- [14]