# Critical magnetic fields in a superconductor coupled to a superfluid

**Authors:** Alexander Haber, Andreas Schmitt

arXiv: 1704.01575 · 2017-07-05

## TL;DR

This paper investigates how coupling a superconductor to a superfluid affects its magnetic properties, revealing a shift in phase transition types and the potential for flux tube clustering, relevant for neutron star cores.

## Contribution

It introduces a temperature-dependent Ginzburg-Landau model for coupled superfluid-superconductor systems and analyzes the impact on critical magnetic fields and phase transitions.

## Key findings

- Transition regions between type-I and type-II become first order due to superfluid coupling.
- Presence of superfluid alters the nature of phase transitions at critical magnetic fields.
- Flux tube clustering may occur in neutron star cores with coupled superfluid and superconductor.

## Abstract

We study a superconductor that is coupled to a superfluid via density and derivative couplings. Starting from a Lagrangian for two complex scalar fields, we derive a temperature-dependent Ginzburg-Landau potential, which is then used to compute the phase diagram at nonzero temperature and external magnetic field. This includes the calculation of the critical magnetic fields for the transition to an array of magnetic flux tubes, based on an approximation for the interaction between the flux tubes. We find that the transition region between type-I and type-II superconductivity changes qualitatively due to the presence of the superfluid: the phase transitions at the upper and lower critical fields in the type-II regime become first order, opening the possibility of clustered flux tube phases. These flux tube clusters may be realized in the core of neutron stars, where superconducting protons are expected to be coupled to superfluid neutrons.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/1704.01575/full.md

## References

52 references — full list in the complete paper: https://tomesphere.com/paper/1704.01575/full.md

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Source: https://tomesphere.com/paper/1704.01575