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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
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.
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
Linking options:
https://www.mathnet.ru/eng/ufn7990 https://www.mathnet.ru/eng/ufn/v152/i4/p683
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