2015/02/28 by J. Clarke, Jackson D. Clarke, R. Foot +2 · 6 citations
Physics and Astronomy · #Baryogenesis #Dark Matter and Cosmic Phenomena #Electroweak interaction #Leptogenesis #Lepton #Naturalness #Neutrino #Neutrino Physics Research #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Seesaw mechanism #Seesaw molecular geometry #Type (biology) #hep-ph
paper · pdf · doi:10.1103/physrevd.91.073009
published as Phys. Rev. D 91, 073009 (2015) · 4 pages, 3 figures, v2 minor changes
openalex publication_date 2015/04/10 · arxiv created 2015/04/13 · arxiv updated 2015/04/16 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04
In the type I seesaw model, the naturalness requirement that corrections to the electroweak \ensuremathμ parameter not exceed 1 TeV results in a rough bound on the lightest right-handed neutrino mass, M_N1\ensuremath\lesssim3\ifmmode×\else\texttimes\fi107 GeV. In this paper we derive generic bounds applicable in any three-flavor type I seesaw model. We find M_N1\ensuremath\lesssim4\ifmmode×\else\texttimes\fi107 GeV and M_N2\ensuremath\lesssim7\ifmmode×\else\texttimes\fi107 GeV. In the limit of one massless neutrino, there is no naturalness bound on M_N3 in the Poincar'e protected decoupling limit. Our results confirm that no type I seesaw model can explain the observed neutrino masses and baryogenesis via hierarchical (N1-, N2-, or N3-dominated) thermal leptogenesis while remaining completely natural.