Physics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pip..work...23e&link_type=abstract
Presented at the Physics of Isolated Pulsars Workshop, Taos, NM, 23-28 Feb. 1992
Physics
Dynamic Characteristics, Neutron Stars, Neutrons, Stellar Composition, Stellar Evolution, Stellar Rotation, Superfluidity, Magnetic Stars, Stellar Temperature
Scientific paper
Neutron superfluid dynamics and the coupling between the superfluid and
the solid crust play important roles in the rotational, thermal, and
magnetic evolution of neutron stars. Here we describe the physical
processes by which the neutron superfluid and the crust interact.
Baym Gordon
Epstein Richard I.
Link Bennett
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