2017
DOI: 10.1142/s0217732317400077
|View full text |Cite
|
Sign up to set email alerts
|

Heavy right-handed neutrino dark matter in left–right models

Abstract: We show that in a class of non-supersymmetric left-right extensions of the Standard Model (SM), the lightest right-handed neutrino (RHN) can play the role of thermal Dark Matter (DM) in the Universe for a wide mass range from TeV to PeV. Our model is based on the gauge groupwhich a heavy copy of the SM fermions are introduced and the stability of the RHN DM is guaranteed by an automatic Z 2 symmetry present in the leptonic sector. In such models the active neutrino masses are obtained via the type-II seesaw me… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

2
20
0

Year Published

2018
2018
2022
2022

Publication Types

Select...
7

Relationship

4
3

Authors

Journals

citations
Cited by 25 publications
(22 citation statements)
references
References 39 publications
2
20
0
Order By: Relevance
“…We then have non-trivial chiral structure of neutral gauge boson interactions with the SM fermions taking into account mixing among neutral gauge bosons. Also models with SU(2) L ×SU (2) gauge extension give two extra neutral gauge bosons in which right-handed partner of the SM fermions are introduced [16][17][18]; similar structure is also found in a model in ref. [19] .…”
Section: Introductionsupporting
confidence: 68%
“…We then have non-trivial chiral structure of neutral gauge boson interactions with the SM fermions taking into account mixing among neutral gauge bosons. Also models with SU(2) L ×SU (2) gauge extension give two extra neutral gauge bosons in which right-handed partner of the SM fermions are introduced [16][17][18]; similar structure is also found in a model in ref. [19] .…”
Section: Introductionsupporting
confidence: 68%
“…Though we focus on the minimal U (1) B−L and LRSM gauge groups in this paper, the basic arguments and main results could easily be generalized to other gauge groups at the TeV scale, such as the SU [49][50][51][52][53], and alternative left-right models with universal seesaw mechanism for the SM quarks and charged leptons [54][55][56][57][58][59][60][61][62][63] or with a stable right-handed neutrino (RHN) dark matter [64,65]. However, our results do not apply to situations where the extra U (1) groups emerge out of non-Abelian groups at an intermediate scale, since they will completely alter the ultraviolet (UV) behavior of the TeV scale U (1) gauge couplings.…”
Section: Introductionmentioning
confidence: 99%
“…From eq. (3.4), we find that the annihilation rate decreases with increasing DM mass, which leads to the unitarity bound of ∼ 20 TeV in our model [93]. Our goal in this subsection is to point out that in our model, there is a way to relax this generic bound without resorting to fine tuning of parameters (as required, e.g.…”
Section: Going Beyond the Unitarity Boundmentioning
confidence: 67%
“…There is also some dilution of DM relic density due to increase in entropy at the QCD phase transition point. Overall, it is possible to get a total dilution factor as big as d ∼ 10 6 , which can relax the unitarity bound for M N up to a PeV or so [93].…”
Section: Jhep11(2016)077mentioning
confidence: 99%