Physics
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phrvc..78a5805z&link_type=abstract
Physical Review C, vol. 78, Issue 1, id. 015805
Physics
4
Equations Of State Of Neutron-Star Matter, Nuclear Matter, Many-Body Theory, Forces In Hadronic Systems And Effective Interactions
Scientific paper
We investigate the effect of microscopic three-body forces on the P3 F2 neutron superfluidity in neutron matter, β-stable neutron star matter, and neutron stars by using the BCS theory and the Brueckner-Hartree-Fock approach. We adopt the Argonne V18 potential supplemented with a microscopic three-body force as the realistic nucleon-nucleon interaction. We have concentrated on studying the three-body force effect on the P3 F2 neutron pairing gap. It is found that the three-body force effect considerably enhances the P3 F2 neutron superfluidity in neutron star matter and neutron stars.
Cui C. X.
Lombardo Umberto
Schulze Hans-Josef
Zuo Wei
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