Time-dependent extension of the self-consistent band theory for neutron star matter: Anti-entrainment effects in the slab phase
Kazuyuki Sekizawa, Sorataka Kobayashi, and Masayuki Matsuo

TL;DR
This paper develops a time-dependent, self-consistent band theory framework to study neutron star crust matter, revealing an anti-entrainment effect where dripped neutrons counterflow, reducing collective mass and increasing conduction neutrons.
Contribution
It introduces the first time-dependent self-consistent band theory application to nuclear matter, specifically analyzing dynamic responses and anti-entrainment effects in neutron star crusts.
Findings
Reduced collective mass due to counterflow of neutrons
Identification of anti-entrainment effect in slab phase
Consistency with static band theory results
Abstract
Background: In the solid crust of neutron stars, a variety of crystalline structure may exist. Recently the band theory of solids has been applied to the inner crust of neutron stars and significance of the entrainment between dripped neutrons and the solid crust was advocated. Since it influences interpretations of various phenomena of neutron stars, it has been desired to develop deeper understanding of the microphysics behind. Purpose: The purpose of the present article is to propose a fully self-consistent microscopic framework for describing time-dependent dynamics of neutron star matter, which allows us to explore diverse properties of nuclear matter, including the entrainment effect. Results: As the first application of the time-dependent self-consistent band theory for nuclear systems, we investigate the slab phase of nuclear matter with various proton fractions. From a…
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