The superfluid phase transition in pulsars

Details The superfluid phase transition in pulsars The superfluid phase transition in pulsars

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jpha...13.2853g&link_type=abstract

Journal of Physics A - Mathematical and General, vol. 13, Aug. 1980, p. 2853-2856. Science Research Council

Physics

2

Neutron Stars, Pulsars, Stellar Models, Superfluidity, Landau-Ginzburg Equations, P Waves, Phase Transformations, Stellar Magnetic Fields

Scientific paper

Renormalization group equations are derived from the Ginzburg-Landau
free energy for p-wave paired neutron-star matter in the presence of
large magnetic fields. The effect of fluctuations on the nature of the
superfluid phase transition is discussed.

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