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Abstract:
A tantalizing hint of isotropic cosmic birefringence has been found in the EB cross-power spectrum of the cosmic microwave background (CMB) polarization data with a statistical significance of 3σ. A pseudoscalar field coupled to the CMB photons via the Chern-Simons term can explain this observation. The same field may also be responsible for early dark energy (EDE), which alleviates the so-called Hubble tension. Since the EDE field evolves significantly during the recombination epoch, the conventional formula that relates EB to the difference between the E- and B-mode autopower spectra is no longer valid. Solving the Boltzmann equation for polarized photons and the dynamics of the EDE field consistently, we find that currently favored parameter space of the EDE model yields a variety of shapes of the EB spectrum, which can be tested by CMB experiments.
