Search for ultra-light axions with CMB polarization

Abstract

When coupled to electromagnetism via a Chern-Simons interaction, axion-like particles (ALP) produce a rotation of the plane of linear polarization of photons known as cosmic birefringence. Recent measurements of cosmic birefringence obtained from the polarization of the cosmic microwave background (CMB) hint at the existence of an isotropic birefringence angle of $\beta \approx 0.3^{\circ }$, currently excluding $\beta =0$ with a statistical significance of $3.6\sigma$. Were such measurement to be confirmed as a cosmological signal, CMB information alone could constrain the ALP parameter space for masses $m_{\varphi }\lesssim 10^{-27}$eV and axion-photon coupling constants $g_{\varphi \gamma }\gtrsim 10^{-20}$GeV${}^{-1}$.

3 pages, 1 figure. Proceedings of the "The dark matter multi-messenger challenge" Symposia of the 2022 Annual Meeting of the European Astronomical Society. To be published in Memorie della SAIt

Cited by in corpus (1)

• A New Solution for the Observed Isotropic Cosmic Birefringence Angle and its Implications for the Anisotropic Counterpart through a Boltzmann Approach