Statefinder diagnostic and $w-w^{\prime}$ analysis for interacting polytropic gas dark energy model
M. Malekjani, A. Khodam-Mohammadi

TL;DR
This paper analyzes an interacting polytropic gas dark energy model using statefinder and $w-w^{\prime}$ diagnostics, showing how model parameters influence cosmic evolution and how it compares to the standard $\Lambda$CDM model.
Contribution
It introduces a detailed diagnostic analysis of the interacting polytropic gas dark energy model, highlighting parameter effects on cosmic evolution trajectories.
Findings
Different parameters lead to distinct evolutionary trajectories in diagnostic planes.
The model mimics the $\Lambda$CDM model at early times.
Parameter variations affect the interaction dynamics.
Abstract
The interacting polytropic gas dark energy model is investigated from the viewpoint of statefinder diagnostic tool and analysis. The dependency of the statefinder parameters on the parameter of the model as well as the interaction parameter between dark matter and dark energy is calculated. We show that different values of the parameters of model and different values of interaction parameter result different evolutionary trajectories in and planes. The polytropic gas model of dark energy mimics the standard CDM model at the early time.
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