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A novel mechanism for kaon condensation in neutron star matter

✍ Scribed by G.E. Brown; Kuniharu Kubodera; Mannque Rho; Vesteinn Thorsson

Publisher
Elsevier Science
Year
1992
Tongue
English
Weight
509 KB
Volume
291
Category
Article
ISSN
0370-2693

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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