We consider a quintessence model for dark energy interacting with dark matter via a Yukawa interaction. To put constraints on this model we use the cosmic microwave background measurements from the Planck satellite together with baryon acoustic oscillation, type Ia supernovae and H₀ data. We conclude that this is a viable model and an appropriate scalar potential can favor the interacting scenario.
No takes yet. Share an insight, caveat, or question.
Costa et al. (2015) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: