Abstract:
Parametrized nucleon density distributions are widely employed for the calculation of the properties of atomic nuclei and dense inhomogeneous matter in compact stars within the Thomas–Fermi method and its extensions. We show that the use of insufficiently smooth parametrizations may deteriorate the accuracy of this method. We discuss and clarify the smoothness condition using the example of the so-called ‘nuclear pasta’ in the neutron star mantle.
Keywords:
superdense matter, neutron star crust, Thomas–Fermi model, equation of state and phase equilibrium
The work was supported by the Russian Science Foundation, grant no. 22-12-00048, by the FWO (Belgium) and the Fonds de la Recherche Scientifique (Belgium) under the Excellence of Science (EOS) programme (project no. 40007501), and alsofrom the Fonds de la Recherche Scientifique (Belgium) under grant no. IISN 4.4502.19.
Received:June 27, 2024 Revised:November 7, 2024 Accepted: November 13, 2024
Citation:
A. Yu. Potekhin, A. I. Chugunov, N. N. Shchechilin, N. Chamel, “On variational trial functions in extended Thomas–Fermi method”, UFN, 195:7 (2025), 738–746; Phys. Usp., 68:7 (2025), 691–698