scholarly journals Higgs portal dark matter and neutrino mass and mixing with a doubly charged scalar

2017 ◽  
Vol 769 ◽  
pp. 121-128 ◽  
Author(s):  
I.M. Hierro ◽  
S.F. King ◽  
S. Rigolin
2014 ◽  
Vol 29 (10) ◽  
pp. 1450064 ◽  
Author(s):  
Sandy S. C. Law ◽  
Kristian L. McDonald

The complexity of radiative neutrino-mass models can be judged by: (i) whether they require the imposition of ad hoc symmetries, (ii) the number of new multiplets they introduce and (iii) the number of arbitrary parameters that appear. Considering models that do not employ new symmetries, the simplest models have two new multiplets and a minimal number of new parameters. With this in mind, we search for the simplest models of radiative neutrino mass. We are led to two models, containing a real scalar triplet and a charged scalar doublet (respectively), in addition to the charged singlet scalar considered by Zee [h+~(1, 1, 2)]. These models are essentially simplified versions of the Zee model and appear to be the simplest models of radiative neutrino mass. However, despite successfully generating nonzero masses, present-day data is sufficient to rule these simple models out. The Zee and Zee–Babu models therefore remain as the simplest viable models. Moving beyond the minimal cases, we find a new model of two-loop masses that employs the charged doublet Φ~(1, 2, 3) and the doubly-charged scalar k++~(1, 1, 4). This is the sole remaining model that employs only three new noncolored multiplets.


2018 ◽  
Vol 2018 ◽  
pp. 1-11
Author(s):  
Najimuddin Khan

We extend the standard model with three right-handed singlet neutrinos and a real singlet scalar. We impose two Z2 and Z2′ symmetries. We explain the tiny neutrino mass-squared differences with two Z2- and Z2′-even right-handed neutrinos using type I seesaw mechanism. The Z2-odd fermion and the Z2′-odd scalar can both serve as viable dark matter candidates. We identify new regions in the parameter space which are consistent with relic density of the dark matter from recent direct search experiments LUX-2016 and XENON1T-2017 and LHC data.


2021 ◽  
Vol 2021 (3) ◽  
Author(s):  
Aleksandr Azatov ◽  
Miguel Vanvlasselaer ◽  
Wen Yin

Abstract In this paper we present a novel mechanism for producing the observed Dark Matter (DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities can lead to the abundance of DM particles with masses much larger than the scale of the transition. We study this non-thermal production mechanism in the context of a generic phase transition and the electroweak phase transition. The application of the mechanism to the Higgs portal DM as well as the signal in the Stochastic Gravitational Background are discussed.


2021 ◽  
pp. 136609
Author(s):  
Sanjoy Mandal ◽  
Nicolás Rojas ◽  
Rahul Srivastava ◽  
José W.F. Valle

2017 ◽  
Vol 2017 (4) ◽  
Author(s):  
M. K. Parida ◽  
Bidyut Prava Nayak ◽  
Rajesh Satpathy ◽  
Ram Lal Awasthi

2018 ◽  
Vol 98 (7) ◽  
Author(s):  
P. S. Bhupal Dev ◽  
Rabindra N. Mohapatra ◽  
Yongchao Zhang

2018 ◽  
Vol 929 ◽  
pp. 193-206 ◽  
Author(s):  
Takaaki Nomura ◽  
Hiroshi Okada ◽  
Hiroshi Yokoya

2020 ◽  
Vol 805 ◽  
pp. 135427 ◽  
Author(s):  
Giorgio Arcadi ◽  
Abdelhak Djouadi ◽  
Marumi Kado

Sign in / Sign up

Export Citation Format

Share Document