Superfluidity in beta-stable neutron star matter

Details Superfluidity in beta-stable neutron star matter Superfluidity in beta-stable neutron star matter

1996-04-25

arxiv.org/abs/nucl-th/9604041v1

Phys.Rev.Lett.77:1428-1431,1996

Physics

Nuclear Physics

Nuclear Theory

7 pages, RevTex latex style, 3 figs included

Scientific paper

10.1103/PhysRevLett.77.1428

In this work we present results for pairing gaps in $\beta$--stable neutron star matter with electrons and muons using a relativistic Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange models for the nucleon--nucleon interaction. Results are given for superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A comparison is made with recent non--relativistic calculations and the implications for neutron star cooling are discussed.

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