Radiative neutrino masses in the singlet-doublet fermion dark matter model with scalar singlets
arXiv:1504.07892 · doi:10.1103/PhysRevD.92.013005
Abstract
When the singlet-doublet fermion dark matter model is extended with additional --odd real singlet scalars, neutrino masses and mixings can be generated at one-loop level. In this work, we discuss the salient features arising from the combination of the two resulting simplified dark matter models. When the -lightest odd particle is a scalar singlet, could be measurable provided that the singlet-doublet fermion mixing is small enough. In this scenario, also the new decay channels of vector-like fermions into scalars can generate interesting leptonic plus missing transverse energy signals at the LHC. On the other hand, in the case of doublet-like fermion dark matter, scalar coannihilations lead to an increase in the relic density which allow to lower the bound of doublet-like fermion dark matter.
16 pages, 6 figures
References in corpus (14)
- Gauge Singlet Scalars as Cold Dark Matter
- Improved Naturalness with a Heavy Higgs: An Alternative Road to LHC Physics
- micrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model
- The Well-Tempered Neutralino
- Neutrino oscillations refitted
- micrOMEGAs4.1: two dark matter candidates
- Search for direct production of charginos, neutralinos and sleptons in final states with two leptons and missing transverse momentum in pp collisions at sqrt(s) = 8 TeV with the ATLAS detector
- Probing the scotogenic model with lepton flavor violating processes
- The low-scale approach to neutrino masses
- Systematic classification of two-loop realizations of the Weinberg operator
- Dark matter and Higgs boson physics
- Scotogenic Inverse Seesaw Model of Neutrino Mass
- Increasing the Neutralino Relic Abundance with Slepton Coannihilations: Consequences for Indirect Dark Matter Detection
- Dark matter in the supersymmetric radiative seesaw model with an anomalous U(1) symmetry