Phenomenological Relations for Axial Quasi-normal Modes of Neutron Stars with Realistic Equations of State
J. L. Bl\'azquez-Salcedo, L. M. Gonz\'alez-Romero, F. Navarro-L\'erida

TL;DR
This paper investigates axial quasi-normal modes of neutron stars with realistic equations of state, revealing how hyperons affect these modes and providing new phenomenological relations to estimate neutron star properties.
Contribution
The study introduces a novel method using Exterior Complex Scaling and provides new phenomenological relations for neutron star quasi-normal modes considering hyperons.
Findings
w-modes can distinguish hyperonic from non-hyperonic neutron stars
New relation between real and imaginary parts of mode frequencies
Influence of core-crust transition pressure is minimal
Abstract
Here we investigate the axial w quasi-normal modes of neutron stars for several equations of state. In particular, we study the influence of the presence of hyperons in the core of the neutron stars. We have obtained that w-modes can be used to distinguish between neutron stars with hyperons and without hyperons for compact enough stars. We present phenomenological relations for the frequency and damping times with the compactness of the neutron star for wI and wII modes showing the differences of the stars with hyperons in the core. Also, we obtain a new phenomenological relation between the real part and the imaginary part of the frequency of the w quasi-normal modes, which can be used to estimate the central pressure of the neutron stars. We are able to construct explicitly the low compactness limit configuration for which the fundamental wII mode vanishes. Finally, we have studied…
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