Neutron Star Vortex Dynamics and Magnetic Field Decay: Implications for High Density Nuclear Matter
classification
⚛️ nucl-th
astro-phhep-ph
keywords
neutrondensitydynamicsimplicationsmagneticmatterstarvortex
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.