Computing Microwave Background Polarization Power Spectra from Cosmic Birefringence
arXiv:2111.14199 · doi:10.1103/PhysRevD.105.063536
Abstract
We present a new publicly available code, $\texttt{class_rot}$, which modifies to enable fast non-perturbative calculation of cosmic microwave background polarization power spectra due to both isotropic and anisotropic polarization rotation from cosmic birefringence. Cosmic birefringence can arise from new parity-violating physics such as axion dark matter with a Chern-Simons coupling to photons or Faraday rotation due to a primordial magnetic field. Constraints on these effects can be obtained by comparing measurements to precise numerical calculations of the polarization power spectra. We describe the implementation of $\texttt{class_rot}$ in terms of both mathematical formalism and coding architecture. We also provide usage examples and demonstrate the accuracy of the code by comparing with simulations.
arXiv comment6 pages, 2 figures, submitted to PRD
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