• Letter

Screening condition in the core of neutron stars

Dmitry Kobyakov
Phys. Rev. C 108, L062801 – Published 1 December 2023

Abstract

Earlier, the screening condition in neutron star core has been formulated as equality of velocities of superconducting protons and the electrons vp=ue at wave numbers qλ1 (λ is the London penetration depth) and has been used to derive the force exerted by the electrons on a moving flux tube. By calculating the current-current response, I find that vpue for l1<qλ1 (l is the electron mean-free path). I show that at typical realistic parameters the electric field induced by a moving (relative to the electrons) flux tube is not screened by the electron currents. The implication is that the existing picture of the momentum exchange between the electrons and the flux tubes must be reassessed.

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  • Received 22 May 2023
  • Revised 18 October 2023
  • Accepted 13 November 2023

DOI:https://doi.org/10.1103/PhysRevC.108.L062801

©2023 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Dmitry Kobyakov*

  • Institute of Applied Physics of the Russian Academy of Sciences, 603950 Nizhny Novgorod, Russia

  • *dmitry.kobyakov@appl.sci-nnov.ru

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Issue

Vol. 108, Iss. 6 — December 2023

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