For two-fluid neutron–dark-matter stars, the paper claims a rigorous equivalence between the static critical-curve stability criterion and the vanishing of a radial oscillation mode, and maps the resulting stable configurations, including mass–radius twin stars.
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Stability Boundary of Neutron-Dark Matter Mixed Stars
For two-fluid neutron–dark-matter stars, the paper claims a rigorous equivalence between the static critical-curve stability criterion and the vanishing of a radial oscillation mode, and maps the resulting stable configurations, including mass–radius twin stars.