The mean-field theory of superfluid-superconducting vortex states in the outer core of neutron stars
Dmitry Kobyakov

TL;DR
This paper extends mean-field theory to characterize superfluid-superconducting vortex states in neutron star cores, considering pressure and temperature effects, and reveals vortex core sizes and limitations of London's approximation.
Contribution
The work introduces a generalized mean-field model for vortex states in neutron star cores, accounting for differing critical temperatures and pressure dependence of pairing gaps.
Findings
Vortex core size exceeds magnetic penetration depth in the outer core.
Entrainment increases vortex core size and decreases magnetic penetration depth.
London's approximation is invalid for neutron vortices in the outer core.
Abstract
Purpose: Characterize superfluid-superconducting vortex states at arbitrary pressures with , assuming both proton and neutron mean-fields are formed by spin-0 Cooper pairs. Method: The existing mean-field theory is extended to account for . The pressure dependence of the pairing gap energy is quantitatively established on the basis of the effective chiral field theory. To link with , I use the weak-coupling result . A quadratic scaled-temperature () dependence of the thermodynamic magnetic field is postulated in analogy with pure superconductors. The -dependence of the gap is inferred from the many-body approximations for the pure neutron matter. Results: An empirical -dependence for the…
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