Superconducting Superfluids in Neutron Stars

Details Superconducting Superfluids in Neutron Stars Superconducting Superfluids in Neutron Stars

2000-10-05

arxiv.org/abs/astro-ph/0010109v1

Grav.Cosmol.Suppl. 6 (2000) 204-213

Astronomy and Astrophysics

Astrophysics

13 pages Latex. Contrib. to Vortices in Unconventional Superconductors and Superfluids, Dresden, March 2000, ed G. Volovik;

Scientific paper

For treatment of the layers below the crust of a neutron star it is useful to employ a relativistic model involving three independently moving constituents, representing superfluid neutrons, superfluid protons, and degenerate negatively charged leptons. A Kalb Ramond type formulation is used here to develop such a model for the specific purpose of application at the semi macroscopic level characterised by lengthscales that are long compared with the separation between the highly localised and densely packed proton vortices of the Abrikosov type lattice that carries the main part of the magnetic flux, but that are short compared with the separation between the neutron vortices.

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