3P/2/ pairing near the transition temperature in neutron-star matter

Details 3P/2/ pairing near the transition temperature in neutron-star matter 3P/2/ pairing near the transition temperature in neutron-star matter

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phrvd..17.1524s&link_type=abstract

Physical Review D - Particles and Fields, 3rd Series, vol. 17, Mar. 15, 1978, p. 1524-1528.

Astronomy and Astrophysics

Astrophysics

21

Astrophysics, Free Energy, Neutron Stars, Pair Production, Functionals, Transition Temperature

Scientific paper

Minima of the general Ginzburg-Landau functional for 3P(2) pairing are determined. The BCS functional lies in a region of the Ginzburg-Landau parameter space where the free energy is minimized by any unitary order parameter. The strong-coupling corrections to the BCS functional for dense neutron matter are estimated. Using current theoretical values for the transition temperature and Landau parameters, it is found that the strong-coupling functional remains in the same region of parameter space as the BCS functional.

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