Abstract:In this work, we consider an interacting dark-fluid cosmological model in which energy exchange between dark matter and dark energy occurs through diffusion. After solving the background expansion history for a late-time universe, we attempt to constrain the cosmological parameters by comparing simulated values of the model against Supernovae Type 1A data. We consider four different cases and compare them against the ΛCDM model as the "true model". Our results show that the diffusive model in which dark energy… Show more
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