Superfluid cores increase neutron star tidal deformabilities and shift universal relations compared with normal-fluid stars, in a general relativistic two-fluid model with a crust.
Continuity of K03 implies ωe(ν −κ )/ 2rψ + {e(ν −κ )/ 2(ψr )′}′ ω is continuous
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Effect of superfluid matter of neutron star on the tidal deformability
Superfluid cores increase neutron star tidal deformabilities and shift universal relations compared with normal-fluid stars, in a general relativistic two-fluid model with a crust.