2005/11/23 by Shaouly Bar-Shalom, Bar-Shalom, Shaouly, David Atwood +3
Computer Science · Physics and Astronomy · #Artificial intelligence #Computational Physics and Python Applications #Computer science #Cosmology and Gravitation Theories #Electron #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Lepton #Neutrino #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Quark #Similarity (geometry) #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0511282
published in arXiv (Cornell University) (Cornell University) · 4 pages, talk given at the International Europhysics Conference on High Energy Physics, July 21st - 27th 2005, Lisboa, Portugal and at the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, June 12th-17th 2006, Irvine, California, USA
openalex publication_date 2005/11/23 · arxiv created 2006/11/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We examine neutrino oscillations in a two Higgs doublet model (2HDM) in which the second doublet couples only to the third generation right-handed up-fermions, i.e., to tR and to N3 which is the heaviest right-handed Majorana neutrino. The inherently large tan(beta) of this model can naturally account for the large top mass and, based on a quark-lepton similarity ansatz, when embedded into a seesaw mechanism it can also account for the observed neutrino masses and mixing angles giving a very small theta13: -0.017 < theta13 < 0.021 at 99% CL, and a very restrictive prediction for the atmospheric mixing angle: 42.9(deg) < thetaatm < 45.2(deg) at 99% CL. The large value of tan(beta) also sets the mass scale of the heaviest right-handed Majorana neutrino N3 and triggers successful leptogenesis through a CP-asymmetry in the decays of the N1 (lightest right-handed Majorana) which is tan2(beta) enhanced compared to the CP-asymmetry obtained in models for leptogenesis with one Higgs doublet or in the MSSM. This enhancement allows us to relax the lower bound on MN1 and consequently also the lower bound on the reheating temperature of the early universe.