The Galactic interstellar medium has a preferred handedness of magnetic misalignment
Zhiqi Huang

TL;DR
This study investigates the origin of the parity-odd $TB$ polarization signal in Galactic dust emission, providing evidence that the observed signal is unlikely due to random fluctuations and suggesting a preferred handedness in magnetic misalignment.
Contribution
The paper demonstrates that the observed $TB$ signal cannot be explained by symmetric magnetic misalignments, indicating a possible parity-violating physics in the interstellar medium.
Findings
Planck data shows a >10 sigma tension with symmetric misalignment simulations.
Galactic filament misalignment likely has a preferred handedness.
Results challenge the assumption that $TB$ signals are purely due to statistical fluctuations.
Abstract
The Planck mission detected a positive correlation between the intensity () and -mode polarization of the Galactic thermal dust emission. The correlation is a parity-odd signal, whose statistical mean vanishes in models with mirror symmetry. Recent work has shown with strong evidence that local handedness of the misalignment between the dust filaments and the sky-projected magnetic field produces signals. However, it remains unclear whether the observed global signal is caused by statistical fluctuations of magnetic misalignment angles, or whether some parity-violating physics in the interstellar medium sets a preferred misalignment handedness. The present work aims to make a quantitative statement about how confidently the statistical-fluctuation interpretation is ruled out by filament-based simulations of polarized dust emission. We use the publicly available…
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