Linear f(Q) gravity yields a maximum compactness bound depending only on the Vaidya-Tikekar parameter K and produces mass-radius curves that shift toward smaller, more compact stars for larger values of the modification parameter α.
Herrera, Stability of the isotropic pressure condition , Phys
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Physical properties and the maximum compactness bound of a class of compact stars in $f(Q)$ gravity
Linear f(Q) gravity yields a maximum compactness bound depending only on the Vaidya-Tikekar parameter K and produces mass-radius curves that shift toward smaller, more compact stars for larger values of the modification parameter α.