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Dark Matter and the Baryon Asymmetry

Glennys R. Farrar, Gabrijela Zaharijas

TL;DR

This work presents a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryons number created in the big bang and naturally explains the observed OmegaDM approximately 5Omegab.

Abstract

We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number $B_X$, and $σ^{\rm annih}_{\bar{X}} < σ^{\rm annih}_{X} $, the $\bar{X}$'s freeze out at a higher temperature and have a larger relic density than $X$'s. If $m_X \lsi 4.5 B_X $GeV and the annihilation cross sections differ by $\mathcal{O}$(10%) or more, this type of scenario naturally explains the observed $Ω_{DM} \approx 5 Ω_b$. Two concrete examples are given, one of which can be excluded on observational grounds.

Dark Matter and the Baryon Asymmetry

TL;DR

This work presents a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryons number created in the big bang and naturally explains the observed OmegaDM approximately 5Omegab.

Abstract

We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number , and , the 's freeze out at a higher temperature and have a larger relic density than 's. If GeV and the annihilation cross sections differ by (10%) or more, this type of scenario naturally explains the observed . Two concrete examples are given, one of which can be excluded on observational grounds.

Paper Structure

This paper contains 12 equations, 1 table.