A consistent view of interacting dark energy from multiple CMB probes

We analyze a cosmological model featuring an interaction between dark energy and dark matter in light of the measurements of the Cosmic Microwave Background released by three independent experiments: the most recent data by the Planck satellite and the Atacama Cosmology Telescope, and WMAP (9-year data). We show that different combinations of the datasets provide similar results, always favoring an interacting dark sector with a 95% C.L. significance in the majority of the cases. Remarkably, such a preference remains consistent when cross-checked through independent probes, while always yielding a value of the expansion rate H0 consistent with the local distance ladder measurements. We investigate the source of this preference by scrutinizing the angular power spectra of temperature and polarization anisotropies as measured by different experiments.

Automated summary

We analyze a cosmological model with interaction between dark energy and dark matter using data from three independent experiments: Planck, Atacama Cosmology Telescope, and WMAP. Regardless of the combination of datasets, the results consistently support an interacting dark sector with a 95% confidence level. This preference remains consistent when cross-checked with independent probes and yields a value for the expansion rate H0 consistent with local distance ladder measurements.