Impact of the Bose-Einstein density profile on anisotropic compact stars under f (Q) gravity*

Abstract This paper presents an innovative framework for modeling anisotropic compact stars by incorporating the density profile of Bose-Einstein condensate dark matter within the gravity framework. This approach provides new insights into the dynamics of compact stars and the role of dark matter in their structure. We derive the metric potential for compact stellar configurations and calculate the associated unknown parameters. Analyzing the physical properties of the compact star PSR J1614-2230 across various values of k , we find that the derived interior solutions for anisotropic stars satisfy all essential physical conditions, thereby confirming the robustness and stability of the proposed model.