Horizontal gauge symmetry and masses of neutrinos

By T. Yanagida. 2005

1,219 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Oceanography

View Paper: https://www.semanticscholar.org/paper/933e79792564b2d5246991eced1fc72d141f749c

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Citations in the corpus

The Majorana Demonstrator Neutrinoless Double-Beta Decay Experiment (2012, background): “A Majorana mass term provides a natural explanation for the lightness of the SM neutrino via the seesaw mechanism [5, 6].”
Leptogenesis (2008, neutral): “1 Singlet fermions (Type I) In the type I seesaw [18, 19, 21, 22], two or three singlet fermions Ni (sometimes referred to as “righthanded neutrinos”) are added the Standard Model.”
Neutrino non-standard interactions: A status report (2019, background): “the Standard Model (SM) with a number of heavy Majorana neutrinos which consequently generate light neutrino masses via the type I seesaw mechanism [48, 177, 178, 235].”
Higgs potential in the type II seesaw model (2011, background): “th the neutrino sector. Probably, one of the most attractive aspects is the ability to induce naturally the tiny neutrino masses from this new avor physics sector [2]. The celebrated seesaw mechanism [3, 4, 5] relating directly the smallness of the neutrino masses to the presence of a large new scal”
Leptogenesis in the Universe (2012, methodology): “We will consider the classic example of leptogenesis from the lightest right-handed (RH) neutrino N1 (the so-called N1 leptogenesis) in the type-I seesaw model [40, 43, 41, 44] in the single flavour regime.”
Flavor structures of charged fermions and massive neutrinos (2019, methodology): “The SM is extended by introducing three right-handed neutrino fields NαR (for α = e, μ, τ) with a sufficiently high mass scale and allowing for lepton number violation [92, 93, 94, 95, 96, 97].”
Running neutrino mass parameters in see-saw scenarios (2005, neutral): “\[Theta]13[x_]:=MNSParameters[mNu[x],Ye[x]][[1,2]]”
The Role of Sterile Neutrinos in Cosmology and Astrophysics (2008, background): “In this section we discuss in detail how the parameters of the Lagrangian (5) should be chosen so as to explain the BSM phenomena without introducing new physics above the electroweak scale.”
The landscape of QCD axion models (2020, background): “Another example is the type-I seesaw model for neutrino masses which, besides accounting for the suppression of the neutrino mass scale [6–9], can also yield quite naturally a cosmological baryon asymmetry of the correct size [10].”