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Published in 2017 at "Astronomische Nachrichten"
DOI: 10.1002/asna.201713441
Abstract: Although the detailed structure of neutron stars remains unknown, their equilibrium temperatures lie well below the Fermi temperature of dense nuclear matter, suggesting that the nucleons in the stars' core form Cooper pairs and exhibit…
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Keywords:
star cores;
fluxtube dynamics;
dynamics neutron;
neutron star ... See more keywords