Neutron stars with a Chaplygin dark fluid core and BSR8 or SLy4 hadronic crusts can satisfy NICER and GW170817 constraints, with larger core-crust density jumps increasing radial stability.
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Dark energy effects on realistic neutron stars
Neutron stars with a Chaplygin dark fluid core and BSR8 or SLy4 hadronic crusts can satisfy NICER and GW170817 constraints, with larger core-crust density jumps increasing radial stability.