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- W3157980357 abstract "The I-Love-Q relations are approximate equation-of-state independent relations that connect the moment of inertia, the spin-induced quadrupole moment, and the tidal deformability of neutron stars. In this paper, we study the I-Love-Q relations for superfluid neutron stars for a general relativistic two-fluid model: one fluid being the neutron superfluid and the other a conglomerate of all charged components. We study to what extent the two-fluid dynamics might affect the robustness of the I-Love-Q relations by using a simple two-component polytropic model and a relativistic mean field model with entrainment for the equation-of-state. Our results depend crucially on the spin ratio $Omega_{rm n}/Omega_{rm p}$ between the angular velocities of the neutron superfluid and the normal component. We find that the I-Love-Q relations can still be satisfied to high accuracy for superfluid neutron stars as long as the two fluids are nearly co-rotating $Omega_{rm n}/Omega_{rm p} approx 1$. However, the deviations from the I-Love-Q relations increase as the spin ratio deviates from unity. In particular, the deviation of the Q-Love relation can be as large as $O(10%)$ if $Omega_{rm n}/Omega_{rm p}$ differ from unity by a few tens of percent. As $Omega_{rm n}/Omega_{rm p} approx 1$ is expected for realistic neutron stars, our results suggest that the two-fluid dynamics should not affect the accuracy of any gravitational waveform models for neutron star binaries that employ the relation to connect the spin-induced quadrupole moment and the tidal deformability." @default.
- W3157980357 created "2021-05-10" @default.
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- W3157980357 date "2021-04-20" @default.
- W3157980357 modified "2023-10-15" @default.
- W3157980357 title "The I-Love-Q Relations for Superfluid Neutron Stars" @default.
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- W3157980357 doi "https://doi.org/10.3390/universe7040111" @default.
- W3157980357 hasPublicationYear "2021" @default.
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