A note on the birefringence angle estimation in CMB data analysis
arXiv:1604.05202 · doi:10.1088/1475-7516/2016/05/020
Abstract
Parity violating physics beyond the standard model of particle physics induces a rotation of the linear polarization of photons. This effect, also known as cosmological birefringence (CB), can be tested with the observations of the cosmic microwave background (CMB) anisotropies which are linearly polarized at the level of . In particular CB produces non-null CMB cross correlations between temperature and B mode-polarization, and between E- and B-mode polarization. Here we study the properties of the so called D-estimators, often used to constrain such an effect. After deriving the framework of both frequentist and Bayesian analysis, we discuss the interplay between birefringence and weak-lensing, which, albeit parity conserving, modifies pre-existing TB and EB cross correlation.
12 pages. Accepted for publication in JCAP
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Cited by in corpus (10)
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- Axion Dark Matter Detection with CMB Polarization
- Improved Constraints on Cosmic Birefringence from the WMAP and Planck Cosmic Microwave Background Polarization Data
- The large scale polarization explorer (LSPE) for CMB measurements: performance forecast
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