Probing Axion-Photon conversion via circular polarization imprints in the CMB $V$-mode observations

TL;DR

This paper proposes a novel method to constrain axion-like particles (ALPs) by analyzing circular polarization imprints in the CMB, leveraging axion-photon conversion in primordial magnetic fields to explore new parameter space.

Contribution

It introduces a new observational approach using CMB V-mode polarization measurements to constrain ALP properties and magnetic field conditions in the early universe.

Findings

Current CMB circular polarization data can set new limits on ALP-photon coupling.

Future observations could probe previously unconstrained ALP mass ranges.

Maximally helical magnetic fields enhance the detectability of axion-photon conversion effects.

Abstract

In the presence of a background magnetic field, axions or axion-like particles (ALPs) can be resonantly converted to photons when their mass is nearly equal to the effective photon mass. In this paper, we propose a novel method to constrain the parameter space of ALPs by investigating the resulting imprints of axion-photon conversion in the cosmic microwave background (CMB) observations. We show that a helical magnetic field existing prior to the CMB epoch can generate an excess population of photons carrying net circular polarization due to the axion-photon conversion mechanism. Consequently, current measurements of the angular power spectrum of circular polarization ($V$-mode) in the CMB can be used to constrain the parameter space of ALP mass and its coupling to photons. In the optimistic scenario of a maximally helical magnetic field with strength $\sim {\rm nG}$, we find that CLASS observations at $40 \, {\rm GHz}$ can probe the previously unconstrained regions of axion-photon coupling corresponding to ALP masses in the range $10^{-10}-10^{-8} \, {\rm eV}$.