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Self-consistent band calculation of the slab phase in the neutron-star crust

Yu Kashiwaba and Takashi Nakatsukasa
Phys. Rev. C 100, 035804 – Published 27 September 2019

Abstract

Fully self-consistent band calculation has been performed for slab phase in neutron-star inner crust using the Barcelona-Catania-Paris-Madrid energy density functional. Optimized slab structure is calculated at given baryon density either with fixed proton ratio or with the beta-equilibrium condition. Numerical results indicate neutron band gaps in order of keV to tens of keV, and the mobility of dripped neutrons are enhanced by the Bragg scattering, which leads to the macroscopic effective mass, m¯z*/mn=0.650.75 near the bottom of the inner crust in neutron stars. However, there is an ambiguity for definition of free neutrons, especially very near the critical density between the slab and the uniform phases, which may effectively lead to somewhat larger values of effective mass. We also compare the results of the band calculation with those of the Thomas-Fermi (TF) approximation. The TF approximation becomes invalid at low density and at high proton ratio.

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  • Received 24 April 2019
  • Revised 8 July 2019

DOI:https://doi.org/10.1103/PhysRevC.100.035804

©2019 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsNuclear Physics

Authors & Affiliations

Yu Kashiwaba1,* and Takashi Nakatsukasa2,1,3,†

  • 1Faculty of Pure and Applied Sciences, University of Tsukuba, Tsukuba 305-8577, Japan
  • 2Center for Computational Sciences, University of Tsukuba, Tsukuba 305-8577, Japan
  • 3RIKEN Nishina Center, Wako 351-0198, Japan

  • *kashiwaba@nucl.ph.tsukuba.ac.jp
  • nakatsukasa@nucl.ph.tsukuba.ac.jp

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Issue

Vol. 100, Iss. 3 — September 2019

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