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Equation of state for pion condensed neutron star matter
Authors:C.K. Au
Affiliation:Department of Physics and Astronomy, University of South Carolina, Columbia, South Carolina 29208, USA
Abstract:We include the effect of the Δ-isobar resonance in the equation of state for neutron star matter in the presence of a pion condensate. We find matter undergoing a first order phase transition after a seconf order phase transition at a much lower density.
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