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

We discuss quantized vortices in neutron $^3P_2$ superfluids, which arebelieved to realize in high density neutron matter such as neutron stars. Byusing the Ginzburg-Landau free energy for $^3P_2$ superfluids, we determine theground state in the absence and presence of the external magnetic field, andnumerically construct $^3P_2$ quantized vortices in the absence and presence ofthe external magnetic field along the vortex axis (poloidal) or angulardirection (toroidal). We find in certain situations the spontaneousmagnetization of the vortex core, whose typical magnitude is about $10^{7-8}$Gauss, but the net magnetic field in a neutron star is negligible because ofthe ratio of the vortex core size $\sim 10$fm and the intervortex distance$\sim 10^{-6}$m in a vortex lattice.

Magnetic Properties of Quantized Vortices in Neutron $^3P_2$ Superfluids in Neutron Stars