Testing CMB Anomalies in E-mode Polarization with Current and Future Data
Rui Shi, Tobias A. Marriage, John W. Appel, Charles L. Bennett, David, T. Chuss, Joseph Cleary, Joseph Eimer, Sumit Dahal, Rahul Datta, Francisco, Espinoza, Yunyang Li, Nathan J. Miller, Carolina N\'u\~nez, Ivan L. Padilla,, Matthew A. Petroff, Deniz A. N. Valle

TL;DR
This study assesses how current and future CMB E-mode polarization data can independently verify known temperature anomalies, showing significant potential for improved constraints especially with future experiments like LiteBIRD.
Contribution
It demonstrates that E-mode polarization data can serve as an independent check on CMB anomalies and quantifies the expected improvements with upcoming experiments.
Findings
LiteBIRD can reduce errors on anomaly estimators by factors of 3 to 26.
E-modes provide largely independent verification of temperature anomalies.
Future data can significantly improve the precision of anomaly measurements.
Abstract
In this paper, we explore the power of the cosmic microwave background (CMB) polarization (E-mode) data to corroborate four potential anomalies in CMB temperature data: the lack of large angular-scale correlations, the alignment of the quadrupole and octupole (Q-O), the point-parity asymmetry, and the hemispherical power asymmetry. We use CMB simulations with noise representative of three experiments -- the Planck satellite, the Cosmology Large Angular Scale Surveyor (CLASS), and the LiteBIRD satellite -- to test how current and future data constrain the anomalies. We find the correlation coefficients between temperature and E-mode estimators to be less than , except for the point-parity asymmetry ( for cosmic-variance-limited simulations), confirming that E-modes provide a check on the anomalies that is largely independent of temperature data. Compared to Planck…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Radio Astronomy Observations and Technology
