scholarly journals One-loop neutrino mass model without any additional symmetries

2019 ◽  
Vol 26 ◽  
pp. 100359 ◽  
Author(s):  
Takaaki Nomura ◽  
Hiroshi Okada
2021 ◽  
Vol 2021 (2) ◽  
Author(s):  
Maria Mehmood ◽  
Mansoor Ur Rehman ◽  
Qaisar Shafi

Abstract We explore proton decay in a class of realistic supersymmetric flipped SU(5) models supplemented by a U(1)R symmetry which plays an essential role in implementing hybrid inflation. Two distinct neutrino mass models, based on inverse seesaw and type I seesaw, are identified, with the latter arising from the breaking of U(1)R by nonrenormalizable superpotential terms. Depending on the neutrino mass model an appropriate set of intermediate scale color triplets from the Higgs superfields play a key role in proton decay channels that include p → (e+, μ+) π0, p → (e+, μ+) K0, p →$$ \overline{v}{\pi}^{+} $$ v ¯ π + , and p →$$ \overline{v}{K}^{+} $$ v ¯ K + . We identify regions of the parameter space that yield proton lifetime estimates which are testable at Hyper-Kamiokande and other next generation experiments. We discuss how gauge coupling unification in the presence of intermediate scale particles is realized, and a Z4 symmetry is utilized to show how such intermediate scales can arise in flipped SU(5). Finally, we compare our predictions for proton decay with previous work based on SU(5) and flipped SU(5).


2015 ◽  
Vol 93 (12) ◽  
pp. 1561-1565
Author(s):  
Ng. K. Francis

We construct the neutrino mass models with non-vanishing θ13 and estimate the baryon asymmetry of the universe and subsequently derive the constraints on the inflaton mass and the reheating temperature after inflation. The great discovery of this decade, the detection of Higgs boson of mass 126 GeV and nonzero θ13, makes leptogenesis all the more exciting. Besides, the neutrino mass model is compatible with inflaton mass 1010–1013 GeV corresponding to reheating temperature TR ∼ 105–107 GeV to overcome the gravitino constraint in supersymmetry and big bang nucleosynthesis. When Daya Bay data θ13 ≈ 9° is included in the model, τ predominates over e and μ contributions, which are indeed a good sign. It is shown that neutrino mass models for a successful leptogenesis can be accommodated for a variety of inflationary models with a rather wide ranging inflationary scale.


2016 ◽  
Author(s):  
Sankagiri Umasankar ◽  
Abhish Dev ◽  
P. Ramadevi
Keyword(s):  

2019 ◽  
Vol 943 ◽  
pp. 114621
Author(s):  
Takaaki Nomura ◽  
Hiroshi Okada
Keyword(s):  

2019 ◽  
Vol 949 ◽  
pp. 114802 ◽  
Author(s):  
Haiying Cai ◽  
Takaaki Nomura ◽  
Hiroshi Okada

2017 ◽  
Vol 95 (1) ◽  
Author(s):  
Kingman Cheung ◽  
Takaaki Nomura ◽  
Hiroshi Okada
Keyword(s):  

2001 ◽  
Vol 501 (1-2) ◽  
pp. 115-127 ◽  
Author(s):  
André de Gouvêa ◽  
José W.F. Valle
Keyword(s):  

2017 ◽  
Vol 2017 (03) ◽  
pp. 025-025 ◽  
Author(s):  
Rome Samanta ◽  
Mainak Chakraborty ◽  
Probir Roy ◽  
Ambar Ghosal

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