Superfluidity and Superconductivity in Neutron Stars
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Neutron stars, the compact stellar remnants of core-collapse supernova explosions, are unique cosmic laboratories for exploring novel phases of matter under extreme conditions. In particular, the occurrence of superfluidity and superconductivity in neutron stars will be briefly reviewed.
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Cited by 3 Pith papers
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Superfluid $^3$He aerogel experiments as a laboratory neutron star analogue
Point-vortex simulations of 3He aerogels identify two pinned-vortex regimes (depinning in crust-like, avalanche creation in core-like) proposed as analogues for neutron-star glitch mechanisms.
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Properties of the neutron star crust informed by nuclear structure data
Bayesian NS EoS study using full nuclear posterior distributions and consistent crust modeling finds increased surface thickness and crustal moment of inertia relative to prior work.
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Superfluid $^3$He aerogel experiments as a laboratory neutron star analogue
Point-vortex simulations of 3He aerogels reveal crust-like depinning and core-like avalanche vortex creation that the authors argue can be mapped to neutron-star glitch dynamics.
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