Flux tubes and the type-I/type-II transition in a superconductor coupled to a superfluid
arXiv:0712.1810 · doi:10.1103/PhysRevB.78.024510
Abstract
We analyze magnetic flux tubes at zero temperature in a superconductor that is coupled to a superfluid via both density and gradient (``entrainment'') interactions. The example we have in mind is high-density nuclear matter, which is a proton superconductor and a neutron superfluid, but our treatment is general and simple, modeling the interactions as a Ginzburg-Landau effective theory with four-fermion couplings, including only s-wave pairing. We numerically solve the field equations for flux tubes with an arbitrary number of flux quanta, and compare their energies. This allows us to map the type-I/type-II transition in the superconductor, which occurs at the conventional kappa = 1/sqrt(2) if the condensates are uncoupled. We find that a density coupling between the condensates raises the critical kappa and, for a sufficiently high neutron density, resolves the type-I/type-II transition line into an infinite number of bands corresponding to ``type-II(n)'' phases, in which n, the number of quanta in the favored flux tube, steps from 1 to infinity. For lower neutron density, the coupling creates spinodal regions around the type-I/type-II boundary, in which metastable flux configurations are possible. We find that a gradient coupling between the condensates lowers the critical kappa and creates spinodal regions. These exotic phenomena may not occur in nuclear matter, which is thought to be deep in the type-II region, but might be observed in condensed matter systems.
14 pages, improved discussion of the effects of varying the neutron/proton condensate ratio; added references
References in corpus (3)
Cited by in corpus (22)
- Stability of interlinked neutron vortex and proton flux tube arrays in a neutron star: equilibrium configurations
- Type-1.5 superconductivity in multicomponent systems
- Chiral anomaly induces superconducting baryon crystal
- A Class of Nonperturbative Configurations in Abelian-Higgs Models: Complexity from Dynamical Symmetry Breaking
- Superfluid drag of two-species Bose-Einstein condensates in optical lattices
- Insights into the physics of neutron star interiors from pulsar glitches
- Multiple-q current states in a multicomponent superconducting channel
- Anti-glitches within the standard scenario of pulsar glitches
- Dynamical onset of superconductivity and retention of magnetic fields in cooling neutron stars
- Stability of interlinked neutron vortex and proton flux-tube arrays in a neutron star -- III. Proton feedback
- Dissipationless Vector Drag--Superfluid Spin Hall Effect
- Gapless neutron superfluidity in the crust of the accreting neutron stars KS 1731-260 and MXB 1659-29
- Josephson currents in neutron stars
- On QCD strings beyond non-interacting model
- Fluxtube Dynamics in Neutron Star Cores
- Surface energy of magnetized superconducting matter in the neutron star cores
- Intermediate-Distance String Effects in Wilson Loops\\ via Boundary Action
- Drag-induced dynamical formation of dark solitons in Bose mixture on a ring
- Magnetic field at the center of a vortex: a new criterion for the classification of the superconductors
- Magnetic coupling through flux branching of adjacent type-I and -II superconductors in a neutron star
- Strings of diquark-quark (QQ)Q baryon before phase transition
- Flux tube clustering from magnetic coupling of adjacent type-I and -II superconductors in a neutron star: persistent gravitational radiation