Possible Charged Pion Condensation in Neutron Matter with Small Proton Admixture
Author(s) -
T. Otofuji,
M. Yasuno
Publication year - 1982
Publication title -
progress of theoretical physics
Language(s) - English
Resource type - Journals
eISSN - 1347-4081
pISSN - 0033-068X
DOI - 10.1143/ptp.67.1645
Subject(s) - physics , pion , condensation , proton , phase transition , neutron , nuclear physics , particle physics , instability , phase (matter) , dense matter , neutron star , condensed matter physics , thermodynamics , quantum mechanics
Since Migdal!) and Sawyer-Scalapino ) pointed out the possibility of pion condensation in nuclear matter, it has intensively studied not only on the pionic instability but also on the structure of pion condensed state. ) Possible spin, isospin and space structures of pion condensate were also considered in detail in both pure neutron matter and isosymmetric nuclear matter. 3 ).4) In a realistic neutron star. there exists an admixture of protons, equilibrating with electrons. These protons give rise to the characteristic pion condensate, so-called Jr, +-condensate, above some critical density. Its possibility has originally been suggested by Migdal, Markin and Mishustin in pure neutron matter though much qualitative as follows: even in pure neutron matter (Z = 0) there exists the energy branch of sound (w~+)
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