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.
Chamel, Superfluidity and Superconductivity in Neu- tron Stars, Journal of Astrophysics and Astronomy 38, 43 (2017) , arXiv:1709.07288 [astro-ph.HE]
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abstract
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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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.
- Superfluid $^3$He aerogel experiments as a laboratory neutron star analogue