2020/06/29 by Y. Minami, Yuto Minami, Eiichiro Komatsu +2 · 5 citations
Chemistry · Physics and Astronomy · #Anisotropy #Astronomy #Astrophysics #Birefringence #COSMIC cancer database #Chemistry #Computational physics #Cosmic microwave background #Cosmology and Gravitation Theories #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Microwave #Optics #Physics #Polarization (electrochemistry) #Quantum mechanics #Spectral line #astro-ph.CO
paper · pdf · doi:10.48550/arxiv.2006.15982
published in arXiv (Cornell University) 2020, 103E02 (Cornell University) · 14 pages, 2 figures, 3 tables
arxiv created 2020/06/29 · openalex publication_date 2020/06/29 · arxiv updated 2020/06/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
We develop a strategy to determine the cosmic birefringence and miscalibrated polarization angles simultaneously using the observed EB polarization power spectra of the cosmic microwave background and the Galactic foreground emission. We extend the methodology of Y. Minami et al. (Prog. Theor. Exp. Phys. 2019, 083E02, 2019), which was developed for auto frequency power spectra, by including cross frequency spectra. By fitting one global birefringence angle and independent miscalibration angles at different frequency bands, we determine both angles with significantly smaller uncertainties (by more than a factor of two) compared to the auto spectra.