Cosmic birefringence from a joint analysis of ACT and Planck
Johannes R. Eskilt
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2026-08-06
Updated: 2026-08-10
Comments: 8 pages, 5 figures. The code to reproduce the results of this paper is available at https://github.com/LilleJohs/cosmic-birefringence-planck-act
Code: https://github.com/LilleJohs/cosmic-birefringence-planck-act
License: http://creativecommons.org/licenses/by/4.0/
The gist: Dark matter and dark energy could be ultra-light pseudoscalar fields that couple to electromagnetism through a Chern-Simons term.
Terminology
Abstract
Dark matter and dark energy could be ultra-light pseudoscalar fields that couple to electromagnetism through a Chern-Simons term. This would cause a parity-breaking rotation of the plane of linearly polarized light from the cosmic microwave background, known as cosmic birefringence, which is not predicted by CDM. Recent hints of a non-zero cosmic birefringence angle have been found in both the Planck Data Release 4 and ACT Data Release 6 datasets independently. This work jointly analyzes the polarized maps of both, leveraging the cross-power spectra between the two telescopes. Taking the reported instrumental priors at face value, the joint analysis yields beta = 0.277 plus or minus 0.057, which is non-zero with a statistical significance of 4.8 sigma. A robustness test mitigating contamination from dust emission excludes beta = 0 at 3.5 sigma, and retrieving beta=0 would require both the dust EB modeling and instrumental priors to fail simultaneously. However, unresolved systematics in the data must be understood before we can draw strong cosmological conclusions.
Sources
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- Quintessence and the Rest of the World
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- Statistics of Cosmic Microwave Background Polarization
- Cosmological Signature of New Parity-Violating Interactions
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- Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data
- The Origin of Parity Violation in Polarized Dust Emission and Implications for Cosmic Birefringence
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- The Atacama Cosmology Telescope: DR6 Maps
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