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 explore the theoretical possibility of $^3P_0$ neutron superfluid indilute spin-polarized neutron matter, which may be relevant to the crust regionof a magnetized neutron star. In such a dilute regime where the neutron Fermienergy is less than 1 MeV, the $^1S_0$ neutron superfluid can be suppressed bya strong magnetic field of the compact star. In the low-energy limit relevantfor dilute neutron matter, the $^3P_0$ interaction is stronger than the $^3P_2$one which is believed to induce the triplet superfluid in the core. We presentthe ground-state phase diagram of dilute neutron matter with respect to themagnetic field and numerically estimate the critical temperature of the $^3P_0$neutron superfluid, which is found to exceed $10^7$ K.

Exploring $^3P_0$ Superfluid in Dilute Spin-Polarized Neutron Matter