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Properties of strange quark stars in $f(Q)$ gravity: A baryon number density-dependent perspective
We study anisotropic strange quark stars in $f(Q)$ gravity, incorporating a baryon-number-density-dependent bag function $B(n)$ into the MIT bag equation of state, $p=[ρ-4B(n)]/3$. Motivated by a Woods-Saxon parametrization, the density dependence of $B(n)$ provides a phenomenological description of
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