Darkogenesis

TL;DR

This paper proposes a model where the baryon asymmetry and dark matter density are generated simultaneously through a first order phase transition in the dark sector, linking the two phenomena.

Contribution

It introduces a novel mechanism where dark matter asymmetry is generated in the hidden sector and transferred to baryons, satisfying cosmological constraints.

Findings

Dark matter asymmetry can be generated via a first order phase transition.

The model successfully transfers asymmetry to baryons through different mechanisms.

Cosmological constraints are satisfied in the proposed scenarios.

Abstract

In standard models of baryogenesis and of dark matter, the mechanisms which generate the densities in both sectors are unrelated to each other. In this paper we explore models which generate the baryon asymmetry through the dark matter sector, simultaneously relating the baryon asymmetry to the dark matter density. In the class of models we explore, a dark matter asymmetry is generated in the hidden sector through a first order phase transition. Within the hidden sector, it is easy to achieve a sufficiently strong first order phase transition and large enough $CP $ violation to generate the observed asymmetry. This can happen above or below the electroweak phase transition, but in both cases significantly before the dark matter becomes non-relativistic. We study examples where the Asymmetric Dark Matter density is then transferred to the baryons both through perturbative and non-perturbative communication mechanisms, and show that in both cases cosmological constraints are satisfied while a sufficient baryon asymmetry can be generated.