A propositional model predicts that the coupling parameter of f(R, L_m, T) gravity shifts the inner edge of a gravastar accretion disk and that surface emission could fill in the central shadow.
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Filling the Shadow: A Propositional Model of Gravastar Accretion in $f(R, L_m, T)$ Gravity
A propositional model predicts that the coupling parameter of f(R, L_m, T) gravity shifts the inner edge of a gravastar accretion disk and that surface emission could fill in the central shadow.