Fig. 2.
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Dependence of critical value, λcrit, on relativistic parameter, σ. On the left we demonstrate the behavior for the polytropic index n < 3 and on the right for n > 3. The gray line on the right highlights the restriction λ = 10−46 g cm−3. The configurations for particular polytropic index n can only exist below the corresponding curve λcrit(n; σ).
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