Leptodermic corrections to the TOV equations and nuclear astrophysics within the effective surface approximation
A.G. Magner, S.P. Maydanyuk, A. Bonasera, H. Zheng, T. Depastas, A.I. Levon, U.V. Grygoriev

TL;DR
This paper introduces surface corrections to the TOV equations for neutron stars using a macroscopic liquid drop model, providing analytical solutions that improve understanding of nuclear effects on stellar structure.
Contribution
It extends the TOV equations by incorporating surface gradient terms within the effective surface approximation, offering a more accurate macroscopic model of neutron star structure.
Findings
Derived modified TOV equations with surface corrections.
Analytical solutions to the MTOV equations at first order.
Comparison shows improvements over standard TOV results.
Abstract
The macroscopic model for a neutron star (NS) as a liquid drop at the equilibrium is used to extend the Tolman-Oppenheimer-Volkoff (TOV) equations taking into account the gradient terms responsible for the system surface. The parameters of the Schwarzschild metric in the spherical case are found with these surface corrections to the known leading (zero) order of the leptodermic approximation , where is the NS effective-surface (ES) thickness, and is the effective NS radius. The energy density is considered in a general form including the functions of the particle number density and of its gradient terms. The macroscopic gravitational component of the energy density is taken into account in the simplest form as expansion in powers of , where is the saturation density, up to second order,…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Astro and Planetary Science · Solar and Space Plasma Dynamics
