Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
Rafael J. F. Marcondes, Ricardo C. G. Landim, Andr\'e A. Costa, Bin, Wang, Elcio Abdalla

TL;DR
This paper derives an analytical formula for the growth rate of cosmic structures in a coupled dark energy-dark matter model, enabling comparison with observations to constrain interaction parameters.
Contribution
It provides the first analytic expression for the growth rate in a coupled dark energy model with energy exchange proportional to dark energy density.
Findings
Analytic formula for the growth rate of structures in the interacting model.
The model's predictions can be directly compared with large-scale structure data.
The approach allows constraining dark energy-dark matter interaction parameters.
Abstract
Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is proportional to the dark energy density. We find that the evolution of can be determined analytically once we know the coupling, the dark energy equation of state, the present value of the dark energy density parameter and the current mean amplitude of dark matter fluctuations. After correcting the growth function for the correspondence with the velocity field through the continuity equation in the interacting model, we use our analytic result to compare the model's predictions with large-scale structure observations.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
