Constraints on Cosmic Birefringence from SPIDER, Planck, and ACT observations
Lu Yin, Shuhang Xiong, Joby Kochappan, Bum-Hoon Lee, Tuhin Ghosh

TL;DR
This paper analyzes cosmic birefringence using data from SPIDER, Planck, and ACT, constraining models involving early dark energy and Chern-Simons coupling, and finds a significant detection of polarization rotation.
Contribution
It provides the first combined analysis of multiple CMB experiments to constrain cosmic birefringence and the Chern-Simons coupling, improving the understanding of parity violation in the early universe.
Findings
SPIDER data incompatible with the Chern-Simons coupling model
Planck and ACT data fit the coupling model reasonably well
Combined Planck+ACT data detect a nonzero polarization rotation angle at 7σ significance
Abstract
The Early Dark Energy (EDE) model has been proposed as a candidate mechanism to generate cosmic birefringence through a Chern-Simons coupling between a dynamical scalar field and the cosmic microwave background (CMB) photon. Such birefringence induces a nonzero cross-correlation between the CMB - and -modes, providing a direct observational signature of parity violation. Recent measurements of the and power spectra, however, cannot yet unambiguously separate instrumental miscalibration () from a true cosmic-rotation angle (). For this reason, we perform a model-independent analysis in terms of the total effective rotation angle . We analyze the latest and measurements from the SPIDER, Planck, and ACT experiments and derive constraints on the Chern-Simons coupling constant and on the polarization rotation angle…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
