English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Our recent Newtonian treatment of the smooth-averaged mutual-friction forceacting on the neutron superfluid and locally induced by the pinning ofquantized neutron vortices to proton fluxoids in the outer core of superfluidneutron stars is here adapted to the general-relativistic framework. We showhow the local nonrelativistic motion of individual vortices can be matched tothe global dynamics of the star using the fully 4D covariant Newtonianformalism of Carter & Chamel (2004). We derive all the necessary dynamicalequations for carrying out realistic simulations of superfluid rotating neutronstars in full general relativity, as required for the interpretation of pulsarfrequency glitches. The role of vortex pinning on the global dynamics appearsto be nontrivial.

Vortex pinning in the superfluid core of relativistic neutron stars