Triplet pairing in beta-stable neutron star matter

Details Triplet pairing in beta-stable neutron star matter Triplet pairing in beta-stable neutron star matter

1996-04-23

arxiv.org/abs/nucl-th/9604032v1

Nucl.Phys. A607 (1996) 425-441

Physics

Nuclear Physics

Nuclear Theory

17 pages, Elsevier latex style elsart, 11 figs included

Scientific paper

10.1016/0375-9474(96)00217-5

$^{3}P_{2}$ pairing in neutron matter is investigated using the Bonn potential models. We find pairing energy gaps in pure neutron matter comparable to the results of previous investigators when the attractive tensor coupling is included. However, taking into account that in a neutron star we have matter at $\beta$ equilibrium, we find that the $^{3}P_{2}$-$^{3}F_{2}$ energy gap is reduced considerably.

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