Probing dark matter with future CMB measurements

The annihilation and decay of dark matter (DM) during the dark ages can leave imprints in the cosmic microwave background (CMB) radiation by altering the cosmic reionization process. CMB polarization anisotropy can be sensitive to such energy injection at higher redshift and therefore helps reducing degeneracy between spectral parameters in ACDM and other astrophysical parameters. In light of several upcoming CMB polarization experiments, such as AdvACTPoI, AliCPT, CLASS, Simons Observatory, Simons Array, SPT-3G, we forecast their prospective sensitivity in probing dark matter annihilation and decay signals. We find that future missions have 95% C.L. projected limits on DM decay and annihilation rates to orders of Gamma(chi)(tau(-1)(chi)) similar to 10(-27) s(-1) and /m(chi) similar to 10(-29) cm(3) s(-1) GeV-1, respectively, significantly improving the sensitivity to DM from current experimental bounds.