New interior model of neutron stars
Camilo Posada, Jan Hlad\'ik, Zden\v{e}k Stuchl\'ik

TL;DR
This paper introduces an exact version of the modified Tolman VII model for neutron stars, improving the description of their interior structure and predicting positive tidal Love numbers consistent with realistic neutron star observations.
Contribution
The paper develops an exact numerical solution to Einstein's equations for the MTVII neutron star model, addressing previous limitations and providing more accurate predictions of tidal properties.
Findings
The EMTVII model predicts positive tidal Love numbers across parameter ranges.
The exact solution better matches realistic neutron star energy density profiles.
The model offers improved insights into neutron star interior structure.
Abstract
The Tolman VII solution is considered by some as one of the few analytical solutions to Einstein's equations, which describes approximately well the interior of neutron stars (NSs). This solution is characterized by the mass , radius , and an energy density that varies quadratically with the radial coordinate . Recently, Jiang and Yagi proposed a modification of this solution, the so-called modified Tolman VII (MTVII) solution, by introducing an additional quartic term to the energy density radial profile. The MTVII solution is an approximate solution to Einstein's equation, which includes a new parameter that allows the solution to have a better agreement with the energy density profiles for realistic NSs. Here we consider the MTVII solution, showing that for certain values of the parameter and compactness this solution manifests a region of…
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