Superfluid extension of the self-consistent time-dependent band theory for neutron star matter: Anti-entrainment versus superfluid effects in the slab phase
Kenta Yoshimura, Kazuyuki Sekizawa

TL;DR
This paper develops a self-consistent time-dependent band theory incorporating superfluidity to study neutron star crusts, revealing significant reductions in effective mass and novel superfluid phenomena in the slab phase.
Contribution
It introduces a formalism combining TDDFT with superfluidity for nuclear band theory and applies it to quantify band structure and superfluid effects in neutron star crust models.
Findings
Slab collective mass reduced by 57.5-82.5% due to superfluidity
Anti-entrainment effect enhances conduction neutron density
Identification of superfluid-specific quasiparticle resonances
Abstract
Background: The inner crust of neutron stars consists of a Coulomb lattice of neutron-rich nuclei, immersed in a sea of superfluid neutrons with background relativistic electron gas. A proper quantum mechanical treatment for such a system under a periodic potential is the band theory of solids. The effect of band structure on the effective mass of dripped neutrons, the so-called \textit{entrainment effect}, is currently in a debatable situation, and it has been highly desired to develop a nuclear band theory taking into account neutron superfluidity in a fully self-consistent manner. Purpose: The main purpose of the present work is twofold: 1) to develop a formalism of the time-dependent self-consistent band theory, taking full account of nuclear superfluidity, based on time-dependent density functional theory (TDDFT) extended for superfluid systems, and 2) to quantify the effects of…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Quantum, superfluid, helium dynamics · High-pressure geophysics and materials
