Forecasts for interacting dark energy with time-dependent momentum exchange
Forecasts for interacting dark energy with time-dependent momentum exchange
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 $\xi(z)$ that could help to alleviate the $S_8$ tension. We perform Fisher forecasting and MCMC analysis to constrain the coupling strength of this interaction for different redshift bins $0.0<z<2.1$, using the specifications of upcoming DESI-like surveys. For this analysis, we examine both a model with a constant equation of state $w=-0.9$, as well as a thawing dark energy model with an evolving $w(z)$. We show that, for a constant equation of state, $\xi(z)$ 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 $w(z)$ model.
Nathan Cruickshank、Robert Crittenden、Kazuya Koyama、Marco Bruni
天文学
Nathan Cruickshank,Robert Crittenden,Kazuya Koyama,Marco Bruni.Forecasts for interacting dark energy with time-dependent momentum exchange[EB/OL].(2025-04-04)[2025-04-27].https://arxiv.org/abs/2504.03555.点此复制
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