Neutron stars and equation of state of nuclear matter

Neutron stars are compact objects whose properties depend strongly on the equation of state of the highly compressed nuclear matter. Analysis of the emission from several extraterrestrial sources whose activity is linked with neutron stars made it possible to refine the characteristics of these stars. This refinement in turn made it possible to obtain additional information on the properties of nuclear matter.

PACS: 21.65.+f, 26.60.+c, 97.60.Jd, 97.10.Kc (all)
DOI: 10.1070/PU1987v030n08ABEH002942
URL: https://ufn.ru/en/articles/1987/8/h/
Citation: Beskin V S "Neutron stars and equation of state of nuclear matter" Sov. Phys. Usp. 30 733–736 (1987)

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%0 Journal Article
%T Neutron stars and equation of state of nuclear matter
%A V. S. Beskin
%I Physics-Uspekhi
%D 1987
%J Phys. Usp.
%V 30
%N 8
%P 733-736
%U https://ufn.ru/en/articles/1987/8/h/
%U https://doi.org/10.1070/PU1987v030n08ABEH002942

Оригинал: Бескин В С «Нейтронные звезды и уравнение состояния ядерной материи» УФН 152 683–689 (1987); DOI: 10.3367/UFNr.0152.198708h.0683