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Planck constraints on cross-correlations between anisotropic cosmic birefringence and CMB polarization

M. Bortolami, M. Billi, A. Gruppuso, P. Natoli, L. Pagano

2022Journal of Cosmology and Astroparticle Physics30 citationsDOIOpen Access PDF

Abstract

Abstract Cosmic Birefringence (CB) is the in-vacuo rotation of the linear polarization direction of photons during propagation, caused by parity-violating extensions of Maxwell electromagnetism. We build low resolution CB angle maps using Planck Legacy and NPIPE products and provide for the first time estimates of the cross-correlation spectra C L αE and C L αB between the CB and the CMB polarization fields. We also provide updated CB auto-correlation spectra C L αα as well as the cross-correlation C L αT with the CMB temperature field. We report constraints by defining the scale-invariant amplitudes A αX ≡ L ( L + 1) C L αX /2 π , where X = α, T, E, B , finding no evidence of CB. In particular, we find A αE = (-7.8 ± 5.6) nK deg and A αB = (0.3 ± 4.0) nK deg at 68% C.L..

Topics & Concepts

PhysicsCosmic microwave backgroundPlanckPolarization (electrochemistry)AnisotropyAstrophysicsSpectral lineAmplitudeBirefringenceParticle physicsQuantum mechanicsPhysical chemistryChemistryCosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaDark Matter and Cosmic Phenomena
Planck constraints on cross-correlations between anisotropic cosmic birefringence and CMB polarization | Litcius