Reconciling $S_8$: Insights from Interacting Dark Sectors
Rahul Shah, Purba Mukherjee, Supratik Pal
arXiv:2404.06396v1 Announce Type: new
Abstract: We do a careful investigation of the prospects of dark energy (DE) interacting with cold dark matter (CDM) in alleviating the $S_8$ clustering tension. To this end, we consider various well-known parametrizations of the DE equation of state (EoS), and consider perturbations in both the dark sectors, along with an interaction term. Moreover, we perform a separate study for the phantom and non-phantom regimes. Using CMB, BAO and SNIa datasets, the constraints on the model parameters for each case have been obtained and a generic reduction in the $H_0-sigma_{8,0}$ correlation has been observed, both for constant and dynamical DE EoS. This reduction, coupled with a significant negative correlation between the interaction term and $sigma_{8,0}$, contributes to easing the clustering tension by lowering $sigma_{8,0}$ to somewhere in between the early CMB and late-time clustering measurements for the phantom regime, for almost all the models under consideration. In addition, this is achieved without exacerbating the Hubble tension. In this regard, the CPL and JBP models perform the best in relaxing the $S_8$ tension to $arXiv:2404.06396v1 Announce Type: new
Abstract: We do a careful investigation of the prospects of dark energy (DE) interacting with cold dark matter (CDM) in alleviating the $S_8$ clustering tension. To this end, we consider various well-known parametrizations of the DE equation of state (EoS), and consider perturbations in both the dark sectors, along with an interaction term. Moreover, we perform a separate study for the phantom and non-phantom regimes. Using CMB, BAO and SNIa datasets, the constraints on the model parameters for each case have been obtained and a generic reduction in the $H_0-sigma_{8,0}$ correlation has been observed, both for constant and dynamical DE EoS. This reduction, coupled with a significant negative correlation between the interaction term and $sigma_{8,0}$, contributes to easing the clustering tension by lowering $sigma_{8,0}$ to somewhere in between the early CMB and late-time clustering measurements for the phantom regime, for almost all the models under consideration. In addition, this is achieved without exacerbating the Hubble tension. In this regard, the CPL and JBP models perform the best in relaxing the $S_8$ tension to $