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Neutron stars and equation of state of nuclear matter


Lebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation

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)
BibTexBibNote ® (generic)BibNote ® (RIS)Medline RefWorks
RT Journal
T1 Neutron stars and equation of state of nuclear matter
A1 Beskin,V.S.
PB Physics-Uspekhi
PY 1987
FD 10 Aug, 1987
JF Physics-Uspekhi
JO Phys. Usp.
VO 30
IS 8
SP 733-736
DO 10.1070/PU1987v030n08ABEH002942
LK https://ufn.ru/en/articles/1987/8/h/

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

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