Cosmic Polarization Rotation in view of the Recent CMB experiments

Abstract

The possibility that there is some Cosmic Polarization Rotation (CPR), i.e. that the polarization angle rotates while a photon travels in vacuum over large distances, is important for at least two reasons: first, the polarization angle seems to be the most steady characteristic of photons and, second, CPR would be associated with violations of fundamental physical principles, like the Einstein Equivalence Principle on which all metric theories of gravity are based, including General Relativity, for which we celebrate the Centennial this year 2015. We review here the astrophysical tests which have been carried out to check if CPR exists. These are using the radio and ultraviolet polarization of radio galaxies and the polarization of the cosmic microwave background (both E-mode and B-mode). These tests so far have been negative, leading to upper limits of a couple of degrees on any CPR angle, thereby increasing our confidence in those physical principles and in the resulting theories, including General Relativity. We discuss future prospects in detecting CPR or improving the constraints on it.