  The concept of dark energy can be used as a possible option to prevent the
gravitational collapse of compact objects into singularities. It affects the
universe on the largest scale, as it is responsible for our universe's
accelerated expansion. As a consequence, it seems possible that dark energy
will interact with any compact astrophysical stellar object [Phys. Rev. D 103,
084042 (2021)]. In this work, our prime focus is to develop a simplified model
of a charged strange star coupled to anisotropic dark energy in
Tolman-Kuchowicz spacetime (Tolman, Phys Rev 55:364, 1939; Kuchowicz, Acta Phys
Pol 33:541, 1968) within the context of general relativity. To develop our
model, here we consider a particular 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. respectively. In this context, we initially started with the equation of
state (EoS) to model the dark energy, in which the dark energy density is
proportional to the isotropic perfect fluid matter-energy density. The unknown
constants present in the metric have been calculated by using the
Darmois-Israel condition. We perform an in-depth analysis of the stability and
force equilibrium of our proposed stellar configuration as well as multiple
physical attributes of the model such as metric function, pressure, density,
mass-radius relation, and dark energy parameters by varying dark energy
coupling parameter $\alpha$. Thus after a thorough theoretical analysis, we
found that our proposed model is free from any singularity and also satisfies
all stability criteria to be a stable and physically realistic stellar model.
