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Non-Abelian vector boson as FIMP dark matter

Basabendu Barman, Subhaditya Bhattacharya, Mohammadreza Zakeri

2020Journal of Cosmology and Astroparticle Physics29 citationsDOIOpen Access PDF

Abstract

In this analysis we demonstrate the freeze-in realization of a non-abelian vector boson dark matter (DM). We choose to elaborate an existing $SU(2)_N$ extension ($N$ stands for neutral) of the Standard Model (SM) with an additional $U(1)=S^{'}$ global symmetry, which stabilizes the vector boson ($X,\bar{X}$) as DM through unbroken $S=T_{3N}+S^{'}$ and as lightest odd $S$ particle. The analysis reveals that the contribution to the freeze-in production of DM from the decay of a heavier scalar bidoublet $\zeta_1^{0,\pm} \to \zeta_2^{0,\pm}X$ is important even after the freeze-out of $\zeta_1^{0,\pm}$ in equilibrium with thermal bath. Moreover, the neutral component of $SU(2)_N$ scalar triplet ($\Delta$), responsible for neutrino mass generation in this framework, turns out to serve as additional DMs in the model and offers a multipartite freeze-in DM set up to explore. The allowed parameter space is obtained after estimating constraints from CMB, BBN and AMS-02 bound. This exercise nicely complements the freeze-out realization of ($X,\bar{X}$) as weakly interacting massive particle (WIMP) and distinguishes it through stable charge track signature at collider compared to leptonic signal excess as found in WIMP scenario.

Topics & Concepts

PhysicsDark matterParticle physicsWIMPScalar (mathematics)Scalar bosonNeutrinoMassive particleBosonStandard Model (mathematical formulation)Realization (probability)MAJORANAVector bosonWeakly interacting massive particlesColliderPhysics beyond the Standard ModelYukawa potentialMultipartiteScalar field dark matterParameter spaceElementary particleTheoretical physicsUnparticle physicsParticle physics theoretical and experimental studiesDark Matter and Cosmic PhenomenaComputational Physics and Python Applications
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