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Zero sound in dense neutron matter

✍ Scribed by P. Haensel


Publisher
Elsevier Science
Year
1978
Tongue
English
Weight
558 KB
Volume
298
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