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arXiv · 1708.06138

Statical properties of CMB B-mode polarisation in a partial sky analysis

Larissa Santos·Wen Zhao
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Abstract

Measuring the imprint of primordial gravitational waves in the cosmic microwave background (CMB) polarisation field is one of the main goals in modern cosmology. However, the so called $B$-mode polarisation can be generated by different sources besides the primary one predicted by inflationary theories, known as secondary $B$-mode signal. Among them, CMB lensing and astrophysical foregrounds play an important role. Moreover, a partial sky analysis leads to a leakage between $E$-modes and $B$-modes. In this article, we use the well known Minkowski functionals (MF) statistics to study the significance of this leakage in the CMB lensing $B$-mode signal. We find that the MF can detect the $E$-to-$B$ leakage contamination, thus it should not be neglected in future CMB data analysis.

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Larissa Santos, Wen Zhao. 2017-08-21. Statical properties of CMB B-mode polarisation in a partial sky analysis. https://doi.org/10.1142/s2010194517600102

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