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On “pion condensation in a relativistic field theory and π-p interaction”

✍ Scribed by N.K. Glendenning; P. Hecking

Book ID
113344477
Publisher
Elsevier Science
Year
1982
Tongue
English
Weight
153 KB
Volume
116
Category
Article
ISSN
0370-2693

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✍ N.K Glendenning; B Banerjee; M Gyulassy 📂 Article 📅 1983 🏛 Elsevier Science 🌐 English ⚖ 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