The 4th Workshop on New Physics Opportunities at Neutrino Facilities

N_eff constraints on the Dark Axion Portal

4 Jun 2024, 15:40

20m

Science and Culture Center (IBS)

Contributed talks I

Speaker

Heejoung Hong

Description

Axions and dark photons are common in many extensions of the Standard Model. The dark axion portal—an axion coupling to the dark photon and photon—can significantly modify their phenomenology. We study the cosmological constraints on the dark axion portal from Cosmic Microwave Background (CMB) bounds on the energy density of dark radiation, $\mathrm{\Delta }{N}_{eff}$. By computing the axion-photon-dark photon collision terms and solving the Boltzmann equations including their effects, we find that light axions are generally more constrained by $\mathrm{\Delta }{N}_{eff}$ than from supernova cooling or collider experiments. However, with dark photons at the MeV scale, a window of parameter space is opened up above the supernova limits and below the experimental exclusion, allowing for axion decay constants as low as $f_a\sim {10}^4$ GeV. This region also modifies indirectly the neutrino energy density, thus relaxing the cosmological upper bound on the sum of ne

Presentation materials

Neff_NPN2024.pdf