Modern cosmology faces the mystery of dark matter and dark energy. Parity violation (mirror symmetry breaking) in their interactions could provide new insights. Earlier hints of cosmic birefringence came from WMAP and Planck data, but independent confirmation with other instruments was needed. This work joins studies of CMB polarization, where neighboring papers examined polarization plane rotation in different contexts, from string theory tests to gravitational lensing effects.
The authors used Bayesian analysis of data from the sixth ACT data release (DR6), including EB and TB polarization correlations. To separate the cosmological rotation angle β from instrumental angles $α_i$, they applied priors for $α_i$ derived from the telescope's optical model. They also accounted for possible residual intensity-to-polarization leakage (I→P). The analysis covered five polarization frequency bands at 90, 150, and 220 GHz.
They obtained β = 0.215° ± 0.074° (68% confidence level), which excludes β = 0 at 2.9σ. The result is robust to the choice of priors and to accounting for I→P leakage. It agrees with previous measurements: WMAP+Planck gave β ≈ 0.342° ± 0.09°, and an independent Cosmoglobe analysis gave β ≈ 0.26° ± 0.10°. A joint analysis with WMAP+Planck raises the significance to 4.6σ, but ACT systematics do not yet allow definitive conclusions.
This work provides independent confirmation of cosmic birefringence using a different instrument and method than previous studies. Unlike neighboring works that focused on gravitational lensing effects or galactic dust polarization, this is the first to apply a Bayesian approach with priors from the ACT optical model. This strengthens confidence in the signal, though systematic uncertainties still need investigation.
Definitive confirmation requires experiments with artificial polarization sources, such as BICEP3, CLASS, and the Simons Observatory. These will allow angle calibration without model assumptions. If the signal is confirmed, it would indicate new physics beyond the Standard Model.
The result will impact cosmology and fundamental physics, as parity violation could point to the nature of dark matter and dark energy.
Independent measurements from other telescopes are needed, along with improved control of systematic uncertainties, especially those related to polarization angle calibration.
This work connects to the unresolved problem of the nature of dark matter and dark energy, and to the question of possible fundamental symmetry violations in cosmology.
This section is addressed to the author of the paper and their colleagues. Neighbouring works were found by meaning-based search across our archive, not by word overlap. We do not review: we show the field around the work.
What the work does
The authors analyzed data from the sixth release of the ACT telescope (DR6), using a Bayesian approach with priors for the instrument angles derived from the optical model. They measured the cosmological polarization rotation angle β = 0.215° ± 0.074°, ruling out a null value at the 2.9σ level, and confirmed agreement with previous results from WMAP and Planck.
Where its strength is
Independent confirmation using a different instrument and method, including accounting for systematic effects and I→P leakage, which boosts the reliability of the cosmic birefringence signal.
Where it could go next
Worth trying
Why this may matter
Independent confirmation of cosmic birefringence on a new instrument strengthens confidence in the signal and paves the way for exploring new physics beyond the Standard Model, such as dark energy interacting with the electromagnetic field.
Nearby works in our archive
The archive is sparse around this work: the closest review is only 0.58, against a usual 0.64. It looks like few have drilled nearby.
The rotation angle β ≈ 0.2° is equivalent to a compass needle turning by 12 arcminutes, which is smaller than the apparent size of the Moon (about 30 arcminutes).
In Greg Egan's novel 'Schild's Ladder', a vacuum with unusual properties is considered, where symmetry breaking plays a key role. Cosmic birefringence is a real candidate for such a phenomenon.