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Kaon condensation in hyperonic matter and properties of neutron stars

โœ Scribed by Takumi Muto

Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
181 KB
Volume
754
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