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≈0.30.3em0exfm^-3.
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Baldo et al. (2007) studied this question.
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