Issues

 / 

1987

 / 

August

  

From the current literature


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) MedlineRefWorks
PT Journal Article
TI Neutron stars and equation of state of nuclear matter
AU Beskin V S
FAU Beskin VS
DP 10 Aug, 1987
TA Phys. Usp.
VI 30
IP 8
PG 733-736
RX 10.1070/PU1987v030n08ABEH002942
URL https://ufn.ru/en/articles/1987/8/h/
SO Phys. Usp. 1987 Aug 10;30(8):733-736

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

© 1918–2024 Uspekhi Fizicheskikh Nauk
Email: ufn@ufn.ru Editorial office contacts About the journal Terms and conditions