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We briefly discuss the intriguing case of a phenomenologicalnon-gravitational coupling in the dark sector, where the interaction isparameterized as an energy transfer either from dark matter to dark energy orthe opposite. We show that a non-zero coupling with an energy flow from thelatter to the former leads to a full reconciliation of the tension betweenhigh- and low-redshift observations present in the standard cosmological model.

Constraining the interaction between dark matter and dark energy with CMB data