Superfluid Dynamics in Neutron Star Crusts(Nuclear Astrophysics,New Frontiers in QCD 2010-Exotic Hadron Systems and Dense Matter-)
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概要
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A simple description of superfluid hydrodynamics in the inner crust of a neutron star is given. Particular attention is paid to the effect of the lattice of nuclei on the properties of the superfluid neutrons, and the effects of entrainment, the fact that some fraction of the neutrons are locked to the motion of the protons in nuclei.
- 2010-12-17
著者
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Reddy Sanjay
T2 Ms B283 Los Alamos National Laboratory
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PETHICK C.
The Niels Bohr International Academy, The Niels Bohr Institute
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CHAMEL N.
Institut d'Astronomie et d'Astrophysique
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REDDY Sanjay
T2, MS B283, Los Alamos National Laboratory
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Chamel N.
Institut D'astronomie Et D'astrophysique
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Pethick C.
The Niels Bohr International Academy The Niels Bohr Institute:nordita
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Pethick C.
The Niels Bohr International Academy, The Niels Bohr Institute:NORDITA