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We derive an equation of state (EOS) for strange matter, starting from an interquark potential which (i) has asymptotic freedom built into it, (ii) shows confinement at zero density (ρ B =0) and deconfinement at high ρ B , and (iii) gives a stable configuration for chargeless, β-stable quark matter. This EOS is then used to calculate the structure of Strange Stars, and in particular...
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