\begin{document}${\rm e}^{\lambda}$\end{document} and \begin{document}${\rm e}^{\nu}$\end{document}. We solve this particular differential equation choosing a simple form of generalized gravitational potential \begin{document}$g_{rr}$\end{document} to describe a complete structure of the space-time within the stellar configuration. After determining this space-time geometry for the stellar models, we discuss thermodynamical observables including radial and tangential pressures, matter density, red-shift, velocity of sound, etc., in the stellar models. We also perform a complete graphical analysis, which shows that our models satisfy all the physical and mathematical requirements of ultra-high dense collapsed structures. Further, we discuss the moment of inertia and M-R curve for rotating and non-rotating stars."> Static fluid spheres admitting Karmarkar condition -
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