CMB spectral distortions from an axion-dark photon-photon interaction

Abstract

Abstract The presence of a plethora of light spin 0 and spin 1 fields is motivated in a number of BSM scenarios, such as the axiverse. The study of the interactions of such light bosonic fields with the Standard Model has focused mostly on interactions involving only one such field, such as the axion (ϕ) coupling to photons, $$\phi F\widetilde{F}$$ , or the kinetic mixing between photon and the dark photon, FF D . In this work, we continue the exploration of interactions involving two light BSM fields and the standard model, focusing on the mixed axion-photon-dark-photon interaction $$\phi F{\widetilde{F}}_{D}$$ . If either the axion or dark photon are dark matter, we show that this interaction leads to conversion of the CMB photons into a dark sector particle, leading to a distortion in the CMB spectrum. We present the details of these unique distortion signatures and the resulting constraints on the $$\phi F{\widetilde{F}}_{D}$$ coupling. In particular, we find that for a wide range of masses, the constraints from these effect are stronger than on the more widely studied axion-photon coupling.

Keywords

• Axions and ALPs
• Models for Dark Matter
• Particle Nature of Dark Matter
• Specific BSM Phenomenology