Scotoseesaw model implied by dark right-handed neutrinos
arXiv:2311.09795 · doi:10.1103/PhysRevD.110.115022
Abstract
We find a dark gauge symmetry that transforms nontrivially only for three right-handed neutrinos, . The anomaly cancellation demands that they have a dark charge assigned to , respectively. The dark charge is broken by two units down to a dark parity, i.e. , which stabilizes a dark matter candidate. Interestingly, the model manifestly supplies neutrino masses via joint seesaw and scotogenic mechanisms, called scotoseesaw.
34 pages, 7 figures, 1 table; substantially improved with references added; matches published version in PRD
References in corpus (17)
- First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
- Search for resonant and nonresonant new phenomena in high-mass dilepton final states at 13 TeV
- Gauging U(1) symmetries and the number of right-handed neutrinos
- Search for supersymmetry in final states with two oppositely charged same-flavor leptons and missing transverse momentum in proton-proton collisions at 13 TeV
- Neutrino masses and CDM in a non-supersymmetric model
- On the importance of the 1-loop finite corrections to seesaw neutrino masses
- The simplest scoto-seesaw model: WIMP dark matter phenomenology and Higgs vacuum stability
- The Search for with 10 Sensitivity: the Upgrade of the MEG Experiment
- Predictions from scoto-seesaw with modular symmetry
- Flavour and dark matter in a scoto/type-II seesaw model
- Common origin of and dark matter within the flavor symmetric scoto-seesaw framework
- Discrete dark matter mechanism as the source of neutrino mass scales
- The Scale Invariant Scotogenic Model: Dark Matter and the Scalar Sector
- Dynamical scoto-seesaw mechanism with gauged
- A Scotogenic Model with Two Inert Doublets
- Interpreting dark matter solution for gauge symmetry
- Can the Higgs field feel a dark force?