Pangenesis in a Baryon-Symmetric Universe: Dark and Visible Matter via the Affleck-Dine Mechanism
Nicole F. Bell, Kalliopi Petraki, Ian M. Shoemaker, Raymond R. Volkas

TL;DR
This paper proposes a unified mechanism, based on the Affleck-Dine process, explaining the similar abundances of dark and visible matter through conserved baryon-like charges in both sectors.
Contribution
It introduces a novel model where baryon asymmetry in visible and dark matter arises from symmetry breaking orthogonal to baryon number via the Affleck-Dine mechanism.
Findings
Dark and visible matter asymmetries can originate from vacuum symmetry breaking.
The model ensures stability of both sectors through symmetry restoration.
It provides a unified explanation for matter abundance coincidence.
Abstract
The similarity of the visible and dark matter abundances indicates that they may originate via the same mechanism. If both the dark and the visible matter are charged under a generalized baryon number which remains always conserved, then the asymmetry of the visible sector may be compensated by an asymmetry in the dark sector. We show how the separation of baryonic and antibaryonic charge can originate in the vacuum, via the Affleck-Dine mechanism, due to the breaking of a symmetry orthogonal to the baryon number. Symmetry restoration in the current epoch guarantees the individual stability of the two sectors.
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