Modeling of Charged Compact Star in f (Q) gravity

This study focuses on constructing physical model of spherically symmetric systems incorporating electromagnetic fields within the framework of f (Q) gravity. To achieve this, we derive the field equations corresponding to f (Q) gravity in the presence of anisotropic matter, and then connect the interior space-time with the exterior Reissner Nordstrom metric to determine the constants inherent in the model. In our approach, we adopt an electrical charge distribution characterized by s(r) = Kr3, where K represents the intensity of the charge to manifest the charged properties of matter distributions. To ensure the physical viability of our solution, we rigorously examine the stability using causality conditions. Subsequently, we apply these developed model to study certain well-known compact objects, such as LMC X- 4. The analysis involve plotting various physical parameters against fixed values incorporated in the model, facilitated by computational software like Mathematica.