A consistent, physical, and analytical model for cosmic microwave background observables of reionisation. I. Derivation, constraining power, and detectability of the auto spectra
The epoch of reionisation imprints its history and morphology on the cosmic microwave background temperature and polarisation anisotropies through two effects: the kinetic Sunyaev Zel'dovich (kSZ) effect and Thomson scattering. To perform joint analyses of these observables and put tight constraints on the reionisation...