Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
Larissa Santos, Kai Wang, Yangrui Hu, Wenjuan Fang, Wen Zhao

TL;DR
This study investigates the impact of E-to-B leakage in partial sky surveys on CMB B-mode polarization analysis, revealing that morphological statistics are sensitive to leakage effects, which are crucial for accurate primordial gravitational wave detection.
Contribution
The paper demonstrates that morphological statistical tools can detect E-to-B leakage residuals in CMB polarization maps, highlighting their importance in primordial B-mode signal analysis.
Findings
Leakage effects are negligible in power spectrum, skewness, kurtosis analyses.
Morphological tools detect leakage at high confidence levels.
Leakage significantly contaminates morphological analyses of B-modes.
Abstract
One of the main goals of modern cosmology is to search for primordial gravitational waves by looking on their imprints in the B-type polarization in the cosmic microwave background radiation. However, this signal is contaminated by various sources, including cosmic weak lensing, foreground radiations, instrumental noises, as well as the E-to-B leakage caused by the partial sky surveys, which should be well understood to avoid the misinterpretation of the observed data. In this paper, we adopt the E/B decomposition method suggested by Smith in 2006, and study the imprints of E-to-B leakage residuals in the constructed B-type polarization maps, , by employing various statistical tools. We find that the effects of E-to-B leakage are negligible for the -mode power spectrum, as well as the skewness and kurtosis analyses of -maps. However, if…
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.
