Superfluidity in beta-stable neutron star matter
Phys.Rev.Lett.77:1428-1431,1996 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 ar...
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| Zusammenfassung: | Phys.Rev.Lett.77:1428-1431,1996 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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| DOI: | 10.48550/arxiv.nucl-th/9604041 |