We investigate the effect of the density-dependent proton and neutron gaps on vortex dynamics in neutron stars. We argue that the persistence of neutron star magnetic fields on timescales of $10^9$ y suggests a superconducting gap curve with local maximum at intermediate density. We discuss the implications for exotic core phenomena such as pion/kaon condensation or a transition to quark matter
Aims: To determine whether ``vortex creep'' in neutron stars, the slow motion of neutron vortices wi...
We consider the amplification and transport of a magnetic field in the collapsed core of a massive s...
Realistic values for the pinning energies of vortices in the neutron superfluid expected in the inne...
A microscopic, quantum mechanical model for neutron vortices in the crust of a neutron star is prese...
We study in a fully selfconsistent approach the structure of a vortex in low density superfluid neut...
The microscopic structure of an isolated vortex line in superfluid neutron star matter is studied by...
We consider a mechanism by which most of the magnetic field in the core of a spinning-down neutron s...
We consider the expulsion of proton fluxoids along neutron vortices from the superfluid/superconduct...
The magnetized vortex lines of the 3P2 paired neutron superfluid are effectively pinned by the magne...
If the generally accepted picture that the neutrons and protons in the core of a neutron star will b...
The cores of neutron stars harbor the highest matter densities known to occur in nature, up to sever...
I show that the usual model of the rotational response of a neutron star, which predicts rotation-in...
This thesis studies the implications of cosmic condensates, specifically the dynamics of superfluid ...
A superconductor of paired protons is thought to form in the core of neutron stars soon after their ...
Recently, neutron stars with very strong surface magnetic fields have been suggested as the site for...
Aims: To determine whether ``vortex creep'' in neutron stars, the slow motion of neutron vortices wi...
We consider the amplification and transport of a magnetic field in the collapsed core of a massive s...
Realistic values for the pinning energies of vortices in the neutron superfluid expected in the inne...
A microscopic, quantum mechanical model for neutron vortices in the crust of a neutron star is prese...
We study in a fully selfconsistent approach the structure of a vortex in low density superfluid neut...
The microscopic structure of an isolated vortex line in superfluid neutron star matter is studied by...
We consider a mechanism by which most of the magnetic field in the core of a spinning-down neutron s...
We consider the expulsion of proton fluxoids along neutron vortices from the superfluid/superconduct...
The magnetized vortex lines of the 3P2 paired neutron superfluid are effectively pinned by the magne...
If the generally accepted picture that the neutrons and protons in the core of a neutron star will b...
The cores of neutron stars harbor the highest matter densities known to occur in nature, up to sever...
I show that the usual model of the rotational response of a neutron star, which predicts rotation-in...
This thesis studies the implications of cosmic condensates, specifically the dynamics of superfluid ...
A superconductor of paired protons is thought to form in the core of neutron stars soon after their ...
Recently, neutron stars with very strong surface magnetic fields have been suggested as the site for...
Aims: To determine whether ``vortex creep'' in neutron stars, the slow motion of neutron vortices wi...
We consider the amplification and transport of a magnetic field in the collapsed core of a massive s...
Realistic values for the pinning energies of vortices in the neutron superfluid expected in the inne...