Models of interacting dark energy and dark matter offer a possible solution to cosmological tensions. In this work, we examine a pure momentum-exchange model with a time-dependent coupling strength that could help to alleviate the tension. We perform Fisher forecasting and MCMC analysis to constrain the coupling strength of this interaction for different redshift bins , using the specifications of upcoming DESI-like surveys. For this analysis, we examine both a model with a constant equation of state , as well as a thawing dark energy model with an evolving . We show that, for a constant equation of state, can be well constrained in all redshift bins. However, due to a weaker effect at early times, the constraints are significantly reduced at high redshifts in the case of a thawing model.

生成讲解博客的中文版本

生成AI智能校验的中文版本