Abstract
Cosmological CPT violation will rotate the polarized direction of CMB photons, convert partial CMB E mode into B mode and vice versa. It will generate non-zero EB, TB spectra and change the EE, BB, TE spectra. This phenomenon gives us a way to detect the CPT-violation signature from CMB observations, and also provides a new mechanism to produce B mode polarization. In this paper, we perform a global analysis on tensor-to-scalar ratio and polarization rotation angles based on current CMB datasets with both low (Planck, BICEP2/Keck Array) and high (POLARBEAR, SPTpol, ACTPol). Benefited from the high precision of CMB data, we obtain the isotropic rotation angle at 68% C.L., the variance of the anisotropic rotation angles , the scale invariant power spectrum and at 95% C.L.. Our result shows that with the polarization rotation effect, the 95% upper limit on gets tightened by 17%.
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