Statefinder hierarchy exploration of the extended Ricci dark energy
Fei Yu, Jing-Lei Cui, Jing-Fei Zhang, Xin Zhang

TL;DR
This paper investigates the extended Ricci dark energy model using the statefinder hierarchy and fractional growth parameter, demonstrating how various parameter combinations can distinguish ERDE from the standard $ ext{Lambda}$CDM model across different redshift regions.
Contribution
The study introduces a comprehensive analysis of ERDE using higher-order statefinders and growth parameters, revealing effective parameter combinations for model discrimination.
Findings
$S_3^{(1)}$ effectively differentiates ERDE from $ ext{Lambda}$CDM.
Combinations $ ext{S}_n^{(1)}$ and $ ext{epsilon}$ break degeneracy at high redshift.
$S_3^{(1)}$ is the best discriminator within ERDE and from $ ext{Lambda}$CDM.
Abstract
We apply the statefinder hierarchy plus the fractional growth parameter to explore the extended Ricci dark energy (ERDE) model, in which there are two independent coefficients and . By adjusting them, we plot evolution trajectories of some typical parameters, including Hubble expansion rate , deceleration parameter , the third and fourth order hierarchy and and fractional growth parameter , respectively, as well as several combinations of them. For the case of variable and constant , in the low-redshift region the evolution trajectories of are in high degeneracy and that of separate somewhat. However, the CDM model is confounded with ERDE in both of these two cases. and , especially the former, perform much better. They can differentiate well only varieties of cases within…
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