Constructing stellar solutions with spherical symmetry through quadratic anisotropy in f(Q) gravity

Abstract This article examines anisotropic models to characterize compact stars (CSs) in the context of modified f(Q) gravity theory. To achieve this, we employ the linear functional form $$f(Q) = \alpha Q + \beta $$ f ( Q ) = α Q + β . A physically meaningful metric potential $$g_{rr}$$ g rr is con...

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Bibliographic Details
Main Authors: R. Kumar, S. K. Maurya, A. Errehymy, A. Jaiswal, K. Myrzakulov, S. Sharma
Format: Article
Language:English
Published: SpringerOpen 2025-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-024-13735-0
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