Compact Star Modeling of Durgapal Solution in $$\boldsymbol{f(Q)}$$ Gravity

This study uses a specific ansatz within $$f(Q)$$ gravity theory to examine the characteristics of spherically symmetric anisotropic compact stars. The research aims at enhance comprehension of these atypical entities by examining the physical properties of the compact star model using the Durgapal geometry within the context of $$f(Q)$$ gravity. The $$f(Q)$$ gravity field equations are resolved using the Karmarkar condition, and the physical characteristics such as density and pressure are computed for the resulting solution. The energy criteria are fulfilled, and the TOV equations perform the equilibrium analysis. The physical study indicates that our models meet the requirements for a well-behaved stellar system. This indicates that our solution is suitable for modeling astrophysical objects.