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- W3133487203 abstract "ABSTRACT Our recent Newtonian treatment of the smooth-averaged mutual-friction force acting on the neutron superfluid and locally induced by the pinning of quantized neutron vortices to proton fluxoids in the outer core of superfluid neutron stars is here adapted to the general-relativistic framework. We show how the local non-relativistic motion of individual vortices can be matched to the global dynamics of the star using the fully 4D covariant Newtonian formalism of Carter & Chamel. We derive all the necessary dynamical equations for carrying out realistic simulations of superfluid rotating neutron stars in full general relativity, as required for the interpretation of pulsar frequency glitches. The role of vortex pinning on the global dynamics appears to be non-trivial." @default.
- W3133487203 created "2021-03-01" @default.
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- W3133487203 date "2021-03-05" @default.
- W3133487203 modified "2023-10-16" @default.
- W3133487203 title "Vortex pinning in the superfluid core of relativistic neutron stars" @default.
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- W3133487203 doi "https://doi.org/10.1093/mnras/stab606" @default.
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