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• W3041852498 abstract "The cosmic infrared background (CIB) is slightly polarized. Polarization directions of individual galaxies could be aligned with tidal fields around galaxies, resulting in nonzero CIB polarization. We use a linear intrinsic alignment model to theoretically predict angular correlations of the CIB polarization fluctuations and find that electriclike and curl-like ($B$-mode) polarization modes are equally generated with power four orders of magnitude less than its intensity. The CIB $B$-mode signal is negligible and not a concerning foreground for the inflationary $B$-mode searches at nominal frequencies for cosmic microwave background measurements, but could be detected at submillimetre wavelengths by future space missions." @default.
• W3041852498 created "2020-07-16" @default.
• W3041852498 creator A5042189570 @default.
• W3041852498 creator A5048187778 @default.
• W3041852498 date "2020-07-10" @default.
• W3041852498 modified "2023-10-16" @default.
• W3041852498 title "Polarization of the Cosmic Infrared Background Fluctuations" @default.
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• W3041852498 doi "https://doi.org/10.3847/1538-4357/ab9013" @default.
• W3041852498 hasPublicationYear "2020" @default.
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