Symmetries identified in Einstein-Maxwell and imperfect fluid spacetimes extend to higher curvature spacetimes.
Vortex Creep Against Toroidal Flux Lines, Crustal Entrainment, and Pulsar Glitches
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
abstract
A region of toroidally oriented quantized flux lines must exist in the proton superconductor in the core of the neutron star. This region will be a site of vortex pinning and creep. Entrainment of the neutron superfluid with the crustal lattice leads to a requirement of superfluid moment of inertia associated with vortex creep in excess of the available crustal moment of inertia. This will effect constraints on the equation of state. The toroidal flux region provides the moment of inertia necessary to complement the crust superfluid with postglitch relaxation behavior fitting the observations.
citation-role summary
background 1
citation-polarity summary
years
2026 2verdicts
UNVERDICTED 2roles
background 1polarities
support 1representative citing papers
A review of spin effects, superfluidity, and magnetic fields in neutron matter and their influence on neutron-star structure, superfluid phases, and rotational dynamics.
citing papers explorer
-
New symmetry in higher curvature spacetimes
Symmetries identified in Einstein-Maxwell and imperfect fluid spacetimes extend to higher curvature spacetimes.
-
Spin effects in superfluidity, neutron matter and neutron stars
A review of spin effects, superfluidity, and magnetic fields in neutron matter and their influence on neutron-star structure, superfluid phases, and rotational dynamics.