Baryoid Dark Matter from $\mathbb{Z}_N$ Domain Walls: The $(N-1):1$ origin of the dark matter-baryon coincidence
Yang Bai, Ting-Kuo Chen

TL;DR
This paper explains the dark matter-baryon coincidence through collapsing $ ext{Z}_N$ domain walls forming baryoids, a novel dark matter candidate, with a natural 6:1 energy-density ratio for $N=7$.
Contribution
It introduces baryoids formed from $ ext{Z}_N$ domain walls as a new dark matter candidate and analyzes their properties and phenomenological implications.
Findings
Baryoids have asteroid-scale mass and nuclear-scale energy density.
The collapse of domain walls yields a baryon-number ratio of $(N-1):1$.
The resulting dark matter-to-baryon energy-density ratio is close to 6:1 for $N=7$.
Abstract
We propose an explanation for the dark matter-baryon coincidence based on collapsing domain walls, which form a novel compact baryonic state: the baryoid. A baryoid has an asteroid-scale mass and up-to-nuclear-scale energy density, and can serve as a dark matter candidate. Starting from equal baryon numbers in the domains formed in the early universe, the collapse of the domain walls after the QCD phase transition leads to a baryon-number ratio of between the false- and true-vacuum domains. Since baryons are slightly lighter in the false-vacuum domains than in the true-vacuum domain, the resulting dark matter-to-baryon energy-density ratio is naturally close to, but slightly smaller than, , or for . We calculate the domain-wall dynamics and the efficiency of baryon-number trapping, derive the resulting baryoid properties, and discuss a broad…
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