Extended I-Love relations for slowly rotating neutron stars
J\'er\'emie Gagnon-Bischoff, Stephen R. Green, Philippe Landry,, N\'estor Ortiz

TL;DR
This paper computes four Love numbers for slowly rotating neutron stars with realistic equations of state, discovering nearly equation-of-state independent relations that extend the I-Love-Q universality, enhancing gravitational-wave data analysis.
Contribution
It introduces new calculations of rotational-tidal Love numbers and establishes nearly universal relations linking these to the moment of inertia, broadening the scope of I-Love-Q relations.
Findings
Discovered nearly EOS-independent relations between Love numbers and moment of inertia.
Computed Love numbers for realistic neutron star equations of state.
Confirmed general-relativistic results with post-Newtonian formulas in the weak-field limit.
Abstract
Observations of gravitational waves from inspiralling neutron star binaries---such as GW170817---can be used to constrain the nuclear equation of state by placing bounds on stellar tidal deformability. For slowly rotating neutron stars, the response to a weak quadrupolar tidal field is characterized by four internal-structure-dependent constants called "Love numbers." The tidal Love numbers and measure the tides raised by the gravitoelectric and gravitomagnetic components of the applied field, and the rotational-tidal Love numbers and measure those raised by couplings between the applied field and the neutron star spin. In this work we compute these four Love numbers for perfect fluid neutron stars with realistic equations of state. We discover (nearly) equation-of-state independent relations between the…
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