scholarly journals Comment on “A three-loop radiative neutrino mass model with dark matter” [Phys. Lett. B 741 (2015) 163]

2015 ◽  
Vol 745 ◽  
pp. 56-57 ◽  
Author(s):  
Chao-Qiang Geng ◽  
Da Huang ◽  
Lu-Hsing Tsai
Keyword(s):  
Dark Matter ◽  
Neutrino Mass ◽  
Mass Model

scholarly journals AFFLECK–DINE LEPTOGENESIS IN THE RADIATIVE NEUTRINO MASS MODEL

2011 ◽  
Vol 26 (06) ◽  
pp. 995-1009 ◽  
Author(s):  
H. HIGASHI ◽  
T. ISHIMA ◽  
D. SUEMATSU
Keyword(s):  
Dark Matter ◽  
Neutrino Mass ◽  
Baryon Number ◽  
Lepton Number ◽  
Neutrino Masses ◽  
Alternative Possibility ◽  
Mass Model ◽  
Neutrino Mass Models ◽  
Baryon Number Asymmetry ◽  
The Universe

Radiative neutrino mass models have interesting features, which make it possible to relate neutrino masses to the existence of dark matter. However, the explanation of the baryon number asymmetry in the universe seems to be generally difficult as long as we suppose leptogenesis based on the decay of thermal right-handed neutrinos. Since right-handed neutrinos are assumed to have masses of O(1) TeV in these models, they are too small to generate the sufficient lepton number asymmetry. Here we consider Affleck–Dine leptogenesis in a radiative neutrino mass model by using a famous flat direction LHu as an alternative possibility. The constraint on the reheating temperature could be weaker than the ordinary models. The model explains all the origin of the neutrino masses, the dark matter, and also the baryon number asymmetry in the universe.

scholarly journals A radiative neutrino mass model with SIMP dark matter

2017 ◽  
Vol 2017 (7) ◽  
Author(s):  
Shu-Yu Ho ◽  
Takashi Toma ◽  
Koji Tsumura
Keyword(s):  
Dark Matter ◽  
Neutrino Mass ◽  
Mass Model

scholarly journals A three-loop radiative neutrino mass model with dark matter

2015 ◽  
Vol 741 ◽  
pp. 163-167 ◽  
Author(s):  
Li-Gang Jin ◽  
Rui Tang ◽  
Fei Zhang
Keyword(s):  
Dark Matter ◽  
Neutrino Mass ◽  
Mass Model
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