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Uspekhi Fizicheskikh Nauk, 1987, Volume 152, Number 4, Pages 683–689
DOI: https://doi.org/10.3367/UFNr.0152.198708h.0683 (Mi ufn7990) 		 
This article is cited in 4 scientific papers (total in 4 papers)

FROM THE CURRENT LITERATURE

Neutron stars and equation of state of nuclear matter

V. S. Beskin

P. N. Lebedev Physical Institute, the USSR Academy of Sciences, Moscow
Full-text PDF (189 kB) Citations (4)
DOI: https://doi.org/10.3367/UFNr.0152.198708h.0683
Abstract: 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.
English version:
Physics–Uspekhi, 1987, Volume 30, Issue 8, Pages 733–736
DOI: https://doi.org/10.1070/PU1987v030n08ABEH002942
Document Type: Article
UDC: 524.354.6
PACS: 21.65.+f, 26.60.+c, 97.60.Jd, 97.10.Kc
Language: Russian
Citation: V. S. Beskin, “Neutron stars and equation of state of nuclear matter”, UFN, 152:4 (1987), 683–689; Phys. Usp., 30:8 (1987), 733–736
Citation in format AMSBIB
\Bibitem{Bes87}
\by V.~S.~Beskin
\paper Neutron stars and equation of state of nuclear matter
\jour UFN
\yr 1987
\vol 152
\issue 4
\pages 683--689
\mathnet{http://mi.mathnet.ru/ufn7990}
\crossref{https://doi.org/10.3367/UFNr.0152.198708h.0683}
\transl
\jour Phys. Usp.
\yr 1987
\vol 30
\issue 8
\pages 733--736
\crossref{https://doi.org/10.1070/PU1987v030n08ABEH002942}
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    • This publication is cited in the following 4 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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