Originally Asymmetric Dark Matter
arXiv:1205.2844 · doi:10.1103/PhysRevD.86.063525
Abstract
We propose a scenario with a fermion dark matter, where the dark matter particle used to be the Dirac fermion, but it takes the form of the Majorana fermion at a late time. The relic number density of the dark matter is determined by the dark matter asymmetry generated through the same mechanism as leptogenesis when the dark matter was the Dirac fermion. After efficient dark matter annihilation processes have frozen out, a phase transition of a scalar field takes place and generates Majorana mass terms to turn the dark matter particle into the Majorana fermion. In order to address this scenario in detail, we propose two simple models. The first one is based on the Standard Model (SM) gauge group and the dark matter originates the doublet Dirac fermion, analogous to the Higgsino-like neutralino in supersymmetric models. We estimate the spin-independent/dependent elastic scattering cross sections of this late-time Majorana dark matter with a proton and find the possibility to discover it by the direct and/or indirect dark matter search experiments in the near future. The second model is based on the gauged extension of the SM, where the dark matter is a SM singlet. Although this model is similar to the so-called Higgs portal dark matter scenario, the spin-independent elastic scattering cross section can be large enough to detect this dark matter in future experiments.
24 pages. Final journal version
References in corpus (26)
- Gauge Singlet Scalars as Cold Dark Matter
- Asymmetric Dark Matter
- Implications of LHC searches for Higgs--portal dark matter
- Asymmetric Dark Matter from Leptogenesis
- The Minimal Set of Electroweak Precision Parameters
- Right-handed sneutrino as thermal dark matter
- Aidnogenesis via Leptogenesis and Dark Sphalerons
- Masses of dark matter and neutrino from TeV scale spontaneous breaking
- Testability of Type I Seesaw at the CERN LHC: Revealing the Existence of the B-L Symmetry
- Signatures for right-handed neutrinos at the Large Hadron Collider
- Oscillating Asymmetric Dark Matter
- Neutralino dark matter from heavy axino decay
- Consequences of DM/antiDM Oscillations for Asymmetric WIMP Dark Matter
- Closing in on Asymmetric Dark Matter I: Model independent limits for interactions with quarks
- Axino dark matter from Q-balls in Affleck-Dine baryogenesis and the coincidence problem
- Sterile neutrino dark matter in extension of the standard model and galactic 511 keV line
- Revival of the Thermal Sneutrino Dark Matter
- Regenerating a Symmetry in Asymmetric Dark Matter
- Dark matter in the classically conformal B-L model
- Unparticle Dark Matter
- The GeV-scale dark matter with B-L asymmetry
- Axino warm dark matter and coincidence
- Affleck-Dine dynamics and the dark sector of pangenesis
- Asymmetric Dark Matter from Spontaneous Cogenesis in the Supersymmetric Standard Model
- Supersymmetric minimal B-L model at the TeV scale with right-handed Majorana neutrino dark matter
- Asymmetric Higgsino Dark Matter
Cited by in corpus (13)
- Review of asymmetric dark matter
- Dark Nuclei I: Cosmology and Indirect Detection
- Exothermic Double-Disk Dark Matter
- Right-handed neutrino dark matter under the B-L gauge interaction
- Phenomenology of WIMPy baryogenesis models
- Asymmetric Dark Matter Models in SO(10)
- Isospin violating dark matter being asymmetric
- Baryogenesis via Leptogenesis from Asymmetric Dark Matter and radiatively generated Neutrino mass
- Selfish Dark Matter
- Exodus: Hidden origin of dark matter and baryons
- Secretly Asymmetric Dark Matter
- Baryonic and Leptonic GeV Dark Matter
- Direct signals from electroweak singlets through the Higgs portal