We search for the signature of parity-violating physics in the Cosmic Microwave Background using Planck polarization data from the Public Release 4 (PR4 or NPIPE). For nearly full-sky data, we initially find a birefringence angle β = 0.30 • ± 0.11 • (68% C.L.). We also find that the values of β decrease as we enlarge the Galactic mask, which can be interpreted as the effect of polarized foreground emission. We use two independent approaches to model this effect and mitigate its impact on β. Although results are promising, and the good agreement between both models is encouraging, we do not assign cosmological significance to the measured value of β until we improve our knowledge of the foreground polarization. Acknowledging that the miscalibration of polarization angles is not the only instrumental systematic that can create spurious TB and EB correlations, we also perform a detailed study of NPIPE end-to-end simulations to prove that our measurements of β are not significantly affected by any of the known systematics.
Parity-violating physics in the CMB polarizationTo this day, we only fully understand about 5% of the contents of the Universe, with the remainder of its energy content split into approximately 27% of Dark Matter (DM), and 68% of Dark Energy (DE). Numerous models have been proposed to explain these two dark components, e.g. 1,2 , a wide range of new weakly interacting massive particles, exotic neutrino models, quintessence, and modified gravity models. Some of them, whether be it as a solution for DM or DE, have in common the introduction of a new pseudoscalar field, φ, that changes sign under the inversion of spatial coordinates, φ(− n) = −φ( n), thus violating parity conservation. A particularly interesting candidate that predicts this type of pseudoscalar field are axion-like particles 3 , which, depending on the value of their mass, could act at the same time as a solution for early DE and then behave like DM at later times.An interesting property that these parity-violating pseudoscalar fields have in common is that, if coupled to the electromagnetic tensor, F µν , and its dual, F µν , via a Chern-Simons