Abstract

Composite asymmetric dark matter scenarios naturally explain why the dark matter mass density is comparable with the visible matter mass density. Such scenarios generically require some entropy transfer mechanism below the composite scale; otherwise, their late-time cosmology is incompatible with observations. A tiny kinetic mixing between a dark photon and the visible photon is a promising example of the low-energy portal. In this paper, we demonstrate that grand unifications in the dark and the visible sectors explain the origin of the tiny kinetic mixing. We particularly consider an ultraviolet completion of a simple composite asymmetric dark matter model, where asymmetric dark matter carries a B − L charge. In this setup, the longevity of asymmetric dark matter is explained by the B − L symmetry, while the dark matter asymmetry originates from the B−L asymmetry generated by thermal leptogenesis. In our minimal setup, the Standard Model sector and the dark sector are unified into SU(5)GUT × SU(4)DGUT gauge theories, respectively. This model generates required B − L portal operators while suppressing unwanted higher-dimensional operators that could wash out the generated B − L asymmetry.

Highlights

  • Galaxy-scale issues of structure formation of collisionless cold dark matter while leaves its success at galaxy clusters

  • We demonstrate that grand unifications in the dark and the visible sectors explain the origin of the tiny kinetic mixing

  • The longevity of asymmetric dark matter is explained by the B − L symmetry, while the dark matter asymmetry originates from the B − L asymmetry generated by thermal leptogenesis

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Summary

Simple composite ADM model

We sketch out a composite ADM model and fix our notation. We consider the vector-like two-flavor SU(3)D × U(1)D dynamics proposed in ref. [36]. The generated B −L asymmetry is shared between the dark and the visible sectors through portal operators, Lportal c1yN Λ2MR The mass of ADM particles is determined by the ratio of the asymmetries in the SM and the dark sectors: mDM = 8.5 GeV [36, 72, 73]. It implies that the dark dynamical scale ΛDQCD is an order of magnitude larger than the QCD scale, namely ΛDQCD ∼ 2 GeV. The hierarchy between Λ and Λ′, namely, between the desirable operators and dangerous operators for an ADM scenario, will be understood in a natural way by a UV completion in the dark sector and its symmetry.

Non-supersymmetric realization
Tiny kinetic mixing
Dark matter phenomenology
Remarks
Supersymmetric realization
Lightest supersymmetric particles in two sectros
Conclusion
Full Text
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