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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.

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Fulltext is also available at DOI: 10.1070/PU1987v030n08ABEH002942
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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Оригинал: Бескин В С «Нейтронные звезды и уравнение состояния ядерной материи» УФН 152 683–689 (1987); DOI: 10.3367/UFNr.0152.198708h.0683

References (33) Cited by (4) Similar articles (2) ↓

  1. A.D. Dolgov “The magnetic monopole after its jubileeSov. Phys. Usp. 27 786–789 (1984)
  2. V.V. Brazhkin, A.G. Lyapin “Transformations of C60 fullerite under high-pressure high-temperature conditionsPhys. Usp. 39 837–840 (1996)

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