
TL;DR
This paper introduces a novel asymmetric dark matter scenario where a fermion transitions from a Dirac to a Majorana particle after relic density is set, with models predicting detectable signals in future experiments.
Contribution
It proposes two simple models for asymmetric dark matter that undergo a late-time phase transition to become Majorana fermions, with testable predictions for direct detection.
Findings
Potential for near-future detection via direct and indirect searches.
Models predict sizable elastic scattering cross sections.
Dark matter relic density linked to leptogenesis-like asymmetry.
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…
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