Nuclear pasta onset in neutron star crusts occurs at a quasi-universal filling fraction u_sp ≈ 0.13-0.15, explained by curvature corrections in the liquid-drop model.
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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions
Nuclear pasta onset in neutron star crusts occurs at a quasi-universal filling fraction u_sp ≈ 0.13-0.15, explained by curvature corrections in the liquid-drop model.