Condensed π- Phase in Neutron-Star Matter

Details Condensed π- Phase in Neutron-Star Matter Condensed π- Phase in Neutron-Star Matter

Aug 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvl..29..382s&link_type=abstract

Physical Review Letters, vol. 29, Issue 6, pp. 382-385

Physics

145

Scientific paper

It is argued that at some density, estimated at about 1 baryon/F3, superdense nuclear matter will make a transition to a phase of approximately equal numbers of protons, neutrons, and π- particles, the latter condensed in one or two plane-wave states of momentum ~170 MeVc. These conclusions are based on the conventional theory of the pionnucleon interaction.

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