Constraining exotic high-$z$ reionization histories with Gaussian processes and the cosmic microwave background

The large-angle polarization anisotropies observed in the cosmic microwave background (CMB) are generated by Thomson scattering of CMB photons off free electrons in the post-recombination Universe. In the standard $Λ$ cold dark matter cosmological model, the free electron density becomes large at redshifts $z \lesssim 10$ due to the formation of the first stars, leading to reionization of the intergalactic medium. In this work, we use \emph{Gaussian processes} to give a model-independent reconstruction of the reionization history of the Universe constrained by the \textit{Planck} CMB measurements. This method gives a consistent reconstruction of the standard reionization at $z \lesssim 10$, and strongly constrains any additional high-$z$ reionization. We use our results to construct a new derived parameter expressing the high-$z$ contribution to the CMB optical depth, $τ_{\mathrm{highz}}$. The posterior distribution on $τ_{\mathrm{highz}}$ can be used to set accurate constraints on models for exotic energy injection, which we demonstrate for the case of decaying dark matter with particle mass in the range $\mathcal{O}(1\,\text{MeV})$. A companion paper demonstrates the use of this methodology to test ensembles of multi-axion models. Our results can be recast to different models using the provided data and code: \href{https://github.com/Cheng-Hanyu/CLASS_reio_gpr}{github.com/Cheng-Hanyu/CLASS\_reio\_gpr}.