Baryonic triplet P-wave dominant superfluidity under combined pion condensation with delta-mixing
Abstract
We study baryonic superfluidity under the combined pion condensation with delta-mixing, where both condensates of the neutral and charged pions take place in neutron stars. Outline of formulation treating such superfluidity is presented and energy gap calculations show the possibility that critical temperatures are higher than about 1x109 K.
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