Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. IV. Role of the symmetry energy in pasta phases

N. N. Shchechilin, N. Chamel, and J. M. Pearson
Phys. Rev. C 108, 025805 – Published 10 August 2023

Abstract

Our previous investigation of neutron-star crusts, based on the functional BSk24, led to a substantial reduction of the pasta mantle when Strutinsky integral and pairing corrections were added on top of the fourth-order extended Thomas-Fermi (ETF) method. Here, our earlier calculations are widened to a larger set of functionals within the same family and we find that the microscopic corrections weaken significantly the influence of the symmetry energy. In particular, the correlation observed at the pure ETF level between the density for the onset of pasta formation and the symmetry energy vanishes, not only for the L coefficient but also for the symmetry-energy values at the relevant densities. Moreover, the inclusion of microscopic corrections results in a much lower abundance of pasta for all functionals.

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  • Received 16 May 2023
  • Accepted 17 July 2023

DOI:https://doi.org/10.1103/PhysRevC.108.025805

©2023 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsNuclear Physics

Authors & Affiliations

N. N. Shchechilin1, N. Chamel1, and J. M. Pearson2

  • 1Institut d'Astronomie et d'Astrophysique, CP-226, Université Libre de Bruxelles, 1050 Brussels, Belgium
  • 2Dépt. de Physique, Université de Montréal, Montréal (Québec), H3C 3J7 Canada

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Vol. 108, Iss. 2 — August 2023

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