Minimal dark matter models with radiative neutrino masses: From Lagrangians to observables
arXiv:2003.04157
Abstract
In this master's thesis, the minimal dark matter models with radiative neutrino masses introduced in arXiv:1308.3655 are examined both in general and, using the model T1-3-B () as a representative, in more detail. In the process, it is both shown how such models are built and a numerical analysis tool chain is established, automating as many steps as possible from the very beginning (deriving the Lagrangian from a given field content) to the very end (calculating observables such as the dark matter relic density, the direct detection cross section and the neutrino masses and mixing matrices). As an important result in laying out the mathematical groundwork, a convention for representations of SU(2) is established which, in this form, is not found in previous works. Another major result is the development of the program minimal-lagrangians, whose capabilities are described in the thesis. It is of great use both for the construction of Lagrangians for new models as well their verification or quick surveys. minimal-lagrangians can be applied to any model within the class it is designed to handle, extending its utility far beyond a one-time result that is only obtained for a single model. Finally, the first steps in the analysis of the model T1-3-B () are taken. It is shown that the model can reproduce both the singlet-doublet fermion dark matter model and the inert triplet model in the appropriate limits. Moreover, the neutrino mass matrix is found and it is demonstrated that the model can accommodate current constraints on the neutrino masses. Lastly, the behavior of the dark matter relic density as it depends on the parameter responsible for the generation of neutrino masses is investigated. Further in-depth study of the model T1-3-B () was performed in a separate publication (arXiv:1812.11133).
arXiv comment226 pages, 32 figures; master's thesis at Westfälische Wilhelms-Universität Münster
References in corpus (37)
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
- Verifiable Radiative Seesaw Mechanism of Neutrino Mass and Dark Matter
- Oscillating neutrinos and mu --> e, gamma
- Minimal Dark Matter
- The MSM, Dark Matter and Baryon Asymmetry of the Universe
- micrOMEGAs3.1 : a program for calculating dark matter observables
- micrOMEGAs2.0: a program to calculate the relic density of dark matter in a generic model
- Dark matter direct detection rate in a generic model with micrOMEGAs2.2
- Pathways to Naturally Small Neutrino Masses
- Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matter
- SUSY Les Houches Accord: Interfacing SUSY Spectrum Calculators, Decay Packages, and Event Generators
- micrOMEGAs: Version 1.3
- SUSY Les Houches Accord 2
- LanHEP - a package for the automatic generation of Feynman rules in field theory. Version 3.0
- Singlet-Doublet Dark Matter
- Probing the scotogenic model with lepton flavor violating processes
- Systematic classification of two-loop realizations of the Weinberg operator
- Radiative corrections to electroweak parameters in the Higgs triplet model and implication with the recent Higgs boson searches
- Discrete dark matter
- Neutrino Mass Hierarchy
- Matter parity as the origin of scalar Dark Matter
- Anomaly-Free Dark Matter Models are not so Simple
- A Class of Inert N-tuplet Models with Radiative Neutrino Mass and Dark Matter
- Scotogenic Inverse Seesaw Model of Neutrino Mass
- A minimal model linking two great mysteries: neutrino mass and dark matter
- Radiative Neutrino Mass with Scotogenic Scalar Triplet
- Dark Matter in Inert Triplet Models
- Doubly-charged scalar bosons from the doublet
- Fermionic WIMPs and Vacuum Stability in the Scotogenic Model
- Connecting neutrino physics with dark matter
- Systematic Study of One-Loop Dirac Neutrino Masses and Viable Dark Matter Candidates
- Mixed Inert Scalar Triplet Dark Matter, Radiative Neutrino Masses and Leptogenesis
- Radiative Type III Seesaw Model and its collider phenomenology
- The Inert Zee Model
- Strategies to link tiny neutrino masses with huge missing mass of the Universe
- Signatures of Dark Matter in Inert Triplet Models
- Deviations of exact neutrino textures using radiative neutrino masses