Physics – Nuclear Physics – Nuclear Theory
Scientific paper
1996-02-13
Nucl.Phys. A604 (1996) 466-490
Physics
Nuclear Physics
Nuclear Theory
uuencoded file, 19 pages, 15 figures included
Scientific paper
10.1016/0375-9474(96)00152-2
In this work we calculate neutron and proton energy gaps in neutron star matter, using the Bonn meson--exchange interactions and a model--space approach to the gap equation. This approach allows a consistent calculation of energy gaps and single particle energies with the model--space Brueckner--Hartree--Fock (MBHF) method, without double counting of two--particle correlations. Neutron energy gaps are calculated at zero and finite temperature. Proton energy gaps are calculated at beta equilibrium, and it is shown that the inclusion of muons has a significant effect. The results are compared with those of other works, and the implications for neutron star physics are briefly discussed.
Elgaroy Oystein
Engvik L.
Hjorth-Jensen Morten
Osnes E.
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