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Hot metastable state of abnormal matter in relativistic nuclear field theory

✍ Scribed by Norman K. Glendenning

Publisher
Elsevier Science
Year
1987
Tongue
English
Weight
1003 KB
Volume
469
Category
Article
ISSN
0375-9474

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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