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Dense neutron matter with realistic interactions

✍ Scribed by V.R. Pandharipande


Publisher
Elsevier Science
Year
1971
Tongue
English
Weight
929 KB
Volume
174
Category
Article
ISSN
0375-9474

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We study different stages of the neutron star cooling by computing neutron star properties at various temperatures and entropies using an effective chiral model including hadronic and quark degrees of freedom. Macroscopic properties of the star such as mass and radius are calculated and compared wit