  Dark energy is one of the potential strategies for preventing compact objects
from gravitationally collapsing into singularities. Because it is the cause of
the accelerated expansion of our universe, it has the greatest impact on the
cosmos. Thus, it is plausible that dark energy will interact with any stellar
object that is compact in the universe [\textit{Phys. Rev. D} \textbf{103},
084042 (2021)]. Our main goal in this work is to create a simplified model, in
the Rastall gravitational framework, of a charged strange star coupled to
anisotropic dark energy in Krori-Barua spacetime [\textit{J. Phys. A, Math.
Gen.} \textbf{8}:508, 1975]. Here, we consider a specific strange star object,
Her X-1, with observed values of mass $=(0.85 \pm 0.15)M_{\odot}$ and radius $=
8.1_{-0.41}^{+0.41}$ km., so that we can develop our model. In this context, we
began by modeling dark energy using the equation of state (EoS), in which the
dark energy density is proportional to the isotropic perfect fluid
matter-energy density. The Darmois-Israel condition has been used to calculate
the unknown constants that are present in the metric. We perform a detailed
analysis of the model's physical properties, including the mass-radius
relation, pressure, density, metric function, and dark energy parameters, by
varying the Rastall coupling parameter. We also examine the stability and force
equilibrium of our proposed stellar configuration. Following a comprehensive
theoretical analysis, we discovered that our suggested model is both
singularity-free and meets all stability requirements needed to be a stable,
physically reasonable stellar model.
