Pion Condensation in Nuclear and Neutron Star Matter

Details Pion Condensation in Nuclear and Neutron Star Matter Pion Condensation in Nuclear and Neutron Star Matter

Jun 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973phrvl..30.1340b&link_type=abstract

Physical Review Letters, vol. 30, Issue 26, pp. 1340-1342

Physics

39

Scientific paper

The equilibrium thermodynamic conditions obeyed by a pion condensed system are given. These include the statement that the average spatial currents of conserved quantities must always vanish in the state of lowest free energy, even for π- condensation into a running-wave mode. The physical significance of pion-condensation thresholds is also discussed.

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