Normal and pion-condensed states in neut
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N.K Glendenning; B Banerjee; M Gyulassy
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Article
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1983
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Elsevier Science
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English
β 966 KB
A theory of isospin asymmetric matter and of neutron star matter in particular, which is compatible with bulk nuclear properties, is formulated in the framework of a relativistic field theory and solved in the mean field approximation. The self-consistent conditions defining the u-. w-, K-, and p-f