Why I-Love-Q
Kent Yagi, Leo C. Stein, George Pappas, Nicolas Yunes, Theocharis A., Apostolatos

TL;DR
This paper investigates the origin of universal relations among multipole moments in neutron stars, revealing that the outer-core's properties and approximate self-similarity of isodensity contours are key to this universality.
Contribution
The study identifies the stellar outer-core as crucial for universality and demonstrates how approximate self-similarity of isodensity contours underpins the observed relations.
Findings
Universal relations are dominated by the outer-core density region.
Relaxing self-similarity assumptions destroys the universality.
Eccentricity is roughly constant in relativistic stars, aiding universality.
Abstract
Black holes are said to have no hair because all of their multipole moments can be expressed in terms of just their mass, charge and spin angular momentum. The recent discovery of approximately equation-of-state-independent relations among certain multipole moments in neutron stars suggests that they are also approximately bald. We here explore the yet unknown origin for this universality. First, we investigate which region of the neutron star's interior and of the equation of state is most responsible for the universality. We find that the universal relation between the moment of inertia and the quadrupole moment is dominated by the star's outer-core, a shell of width (50-95)% of the total radius, which corresponds to the density range -g/cm. Second, we study the impact on the universality of approximating stellar isodensity contours as self-similar ellipsoids.…
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