Charged compact stars in f(Q,T) gravity with Bardeen exterior and Finch-Skea interior satisfy energy conditions, TOV equilibrium, and stability criteria based on causality and adiabatic index.
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Analysis of Charged Compact Stars with Bardeen Black Hole in $f(\mathfrak{Q}, \mathcal{T})$ Gravity
Charged compact stars in f(Q,T) gravity with Bardeen exterior and Finch-Skea interior satisfy energy conditions, TOV equilibrium, and stability criteria based on causality and adiabatic index.