Neutron Star Vortex Dynamics and Magnetic Field Decay: Implications for High Density Nuclear Matter

Abstract

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.

Comments: 7 pages, 2 figures, uses LaTeX