Mass-radius relation, moment of inertia, and tidal love numbers of anisotropic neutron stars in f (R,T) gravity
This study investigates the mass-radius relation, moment of inertia, and tidal Love numbers of anisotropic neutron stars within the gravity framework using the Horvat anisotropy model, demonstrating that while both anisotropy and the gravity parameter influence physical properties, the former has a dominant effect, ultimately identifying specific configurations that satisfy observational constraints from GW170817 and GW190814.