Matter-antimatter asymmetry and dark matter stability from baryon number conservation
arXiv:2307.02592 · doi:10.1088/1475-7516/2024/01/028
Abstract
There is currently no evidence for a baryon asymmetry in our Universe. Instead, cosmological observations have only demonstrated the existence of a quark-antiquark asymmetry, which does not necessarily imply a baryon asymmetric Universe, since the baryon number of the dark sector particles is unknown. In this paper we discuss a framework where the total baryon number of the Universe is equal to zero, and where the observed quark-antiquark asymmetry arises from neutron portal interactions with a dark sector fermion that carries baryon number. In order to render a baryon symmetric universe throughout the whole cosmological history, we introduce a complex scalar , with opposite baryon number and with the same initial abundance as . Notably, due to the baryon number conservation, is absolutely stable and could have an abundance today equal to the observed dark matter abundance. Therefore, in this simple framework, the existence of a quark-antiquark asymmetry is intimately related to the existence (and the stability) of dark matter.
arXiv commentCorrected asymmetry dynamics, conclusion unchanged. 15 pages, 5 figures
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