Cosmological Roles of Dark Photons in Axion-induced Electroweak Baryogenesis

TL;DR

This paper investigates how axion interactions with dark photons can influence electroweak baryogenesis, dark matter, and dark radiation, offering new mechanisms and constraints within cosmological models.

Contribution

It introduces the role of dark photon interactions with axions in electroweak baryogenesis and cosmology, highlighting their potential to suppress decay channels, serve as dark matter, or contribute to dark radiation.

Findings

Dark photons can suppress axion decay to SM particles.

Dark photons can be dark matter candidates if massive and stable.

Dark photons can contribute to dark radiation as ultralight particles.

Abstract

By coupling to both the Higgs and electroweak gauge sectors, an axion can generate the matter-antimatter asymmetry in the universe via electroweak baryogenesis when the axion decay constant lies within the range of approximately $10^5$ and $10^7$GeV, corresponding to axion masses between the MeV and GeV scales. In this work, we explore the intriguing possibility that the axion interacts with a dark sector, particularly with dark photons through anomalous couplings. Notably, axion-coupled dark photons can play multiple roles, including $(i)$ suppressing the branching ratio of axion decay to Standard Model (SM) particles, which would otherwise conflict with the constraints from supernovae explosions, Big Bang nucleosynthesis, and neutron star merger events, $(ii)$ serving as a candidate for cold dark matter if they are massive and stable, and $(iii)$ contributing to dark radiation if they are ultralight. The axion decouples from the SM thermal bath when it becomes non-relativistic, facilitating the production of dark matter dark photons through the freeze-in mechanism, while dark radiation dark photons are thermally generated prior to the electroweak phase transition.