Influence of strong-coupling corrections on the equilibrium phase for 3P2 superfluid neutron-star matter

Details Influence of strong-coupling corrections on the equilibrium phase for 3P2 superfluid neutron-star matter Influence of strong-coupling corrections on the equilibrium phase for 3P2 superfluid neutron-star matter

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvd..29.2705v&link_type=abstract

Physical Review D (Particles and Fields), Volume 29, Issue 12, 15 June 1984, pp.2705-2711

Physics

3

Scientific paper

We calculate strong-coupling corrections to the 3P2 neutron-star-matter Ginzburg-Landau functional including spin-orbit and central forces. Based on a two-parameter approximation for the spin-orbit scattering amplitude and typical estimates for the neutron-matter Landau parameters we conclude that the most likely equilibrium phase of 3P2 neutron matter is described by a unitary order parameter. Better calculations of neutron-matter parameters, particularly the spin-orbit scattering amplitude, would allow a stronger conclusion.

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