Physical viability of f(Q) gravity corrected charged anisotropic solutions

Abstract

This article explores the impact of charge on the properties of relativistic compact star candidates exhibiting anisotropic distribution in $f\left(Q\right)$ gravity, where $Q$ represents a nonmetricity. A specific model of this gravitational theory is considered to simplify the system and establish the precise field equations that regulate the interaction between matter and geometry. Analysis of the static spherical symmetric structures is conducted by considering the non-singular feasible solutions. The Darmois constraints are used to determine the unknown constants in the metric coefficients. We explore different physical characteristics in the interior of charged compact stars to check their viability. Sound velocity and adiabatic index techniques are employed for stability state analysis. Proposed charged stars are determined to be both viable and stable in this theoretical framework.