Proton pairing in neutron stars

Physics

Scientific paper

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Nuclear Matter Aspects Of Neutron Stars, Nuclear Matter, Many-Body Theory

Scientific paper

We studied the influence of dispersive self-energy effects, three-body forces, and polarization contributions to the interaction kernel on the 1S0 proton pairing in neutron star matter. We found that a strong suppression of the gap by self-energy effects and three-body forces is at low density compensated by the attractive polarization interaction, shifting the domain of pairing to below ρB≈0.3fm-3.

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