Anisotropic Strange Star Model Beyond Standard Maximum Mass Limit by Gravitational Decoupling in f(Q)$f(Q)$ Gravity

The current theoretical development identified as the gravitational decoupling via Complete Geometric Deformation (CGD) method that has been introduced to explore nonmetricity $Q$ effects in relativistic astrophysics. In present work, we have investigated gravitationally decoupled anisotropic solutions for strange star framework of $f(Q)$ gravity by utilizing CGD technique. To do this, started with Tolman metric ansatz along MIT Bag model equation state related hadronic matter. governing equations motions are obtained using two approaches, namely mimicking $\theta$ sector seed radial pressure and energy density fluid model. models describe self-gravitating static, compact objects whose exterior solution can be given vacuum Schwarzschild Anti-de Sitter spacetime. particular, modeled five stellar candidates, viz., LMC X-4, PSR J1614-2230, J0740+6620, GW190814, GW 170817 observational data. rigorous viability tests performed through regularity stability conditions. We observed parameter constant show a significant effect on stabilizing ensure physically realizable models. innovative feature this work is stable masses beyond $2 M_{\odot}$ without engaging exotic Therefore, study shows new perception physical significance about exploration ultra-compact astrophysical objects.