Testing the Direction of Dark Sector Interaction Using Late-Time Datasets
Using late-time datasets including DESI DR1/DR2, cosmic chronometers, CMB, and various supernova compilations, this study finds that while the interacting dark energy model slightly alleviates the Hubble tension and suggests a weak preference for energy transfer from dark energy to dark matter, the data ultimately provide no statistically significant evidence for dark sector interaction and consistently favor the standard CDM model.