Neutron stars and equation of state of nuclear matter

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

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)

Manchester R and J Taylor Pulsars (Mir, M., 1980)
Shapiro S L and S A Teukolsky Black Holes, White Dwarfs, And Neutron Stars: The Physics Of Compact Objects (Mir., M., 1985)
Ginzburg V L Theoretical Physics And Astrophysics (Nauka, M., 1980)
Oppenheimer J R and G Volkoff Phys. Rev. 55 374 (1939)
Bethe H A "Theory of nuclear matter" Ann. Rev. Nucl. Sci. 21 93 (1971); Russ. transl., Bethe H A Theory Of Nuclear Matter (Mir, M.], 1974)
Dyson F J Neutron Stars And Pulsars: Fermi Lectures, 1970 (Accademia dei Lincei, Roma, 1971); Dyson F J Problemi Attuali Di Scienza E Di Cultura (No. 152) (1972), March; ter Haar D "Pulsars" Phys. Rep. 3C (No. 2) (1972), March; Russian transl. of both, Dyson F J Pulsars (Mir, M.], 1973)
Pandharipande V R, D Pines, and R A Smith Astrophys. J. 208 550 (1976)
Arnett W D and R L Bowers Astrophys. J. Suppl. 33 415 (1977)
Alpar M A P. W. Anderson, D. Pines, And J. Shaham, Astrophys. J. 276 325 (1984)
Flowers E G, J F Lee, M A Ruderman et al Astrophys. J. 215 291 (1977)
Amnu P R él’ The X-ray Sky (In Russian) (Nauka, M., 1984)
Pines D J. Phys. (Paris) C. 2 111 (1980); Pines D Russ. Transl. Usp. Fiz. Nauk 131 479 (1980)
Kirzhnits D A and Yu A Nepomnyashchi&ibreve; Zh. Eksp. Teor. Fiz. 59 2203 (1970)
Migdal A B Fermions And Bosons In Strong Fields (in Russian) (Nauka, M., 1978)
Baym G and C Pethick Ann. Rev. Astron. Astrophys. 17 415 (1979)
Usov V V Scientific And Technological Progress. Vol. 9 (in Russian) (VINITI Akad. SSSR, M., 1977)
Weisberg J M, J H Taylor, and L A Fowler Sci. Am. 245 (4) 74 (1982), Oct.; Russ. transl., Weisberg J M, J H Taylor, and L A Fowler Usp. Fiz. Nauk 137 707 (1982)
Backer D C and R W Hellings Ann. Rev. Astron. Astrophys. 24 537 (1986)
Joss P C and S A Rappaport Ann. Rev. Astron. Astrophys. 22 537 (1984)
Shapiro S L, S A Teukolsky, and I Wasserman Astrophys. 272 702 (1983)
Fujimoto M Y Astrophys. 293 L19 (1985)
Lindblom L Astrophys. 303 146 (1986)
Liang E P Astrophys. 304 682 (1986)
Fujimoto M Y and R E Taam Astrophys. 305 246 (1986)
Sztaino M, M Y Fujimoto, J van Paradijs et al Mon. Not. R. Astron. Soc. 226 39 (1986)
Mazets E P and S V Golenetski&ibreve; Astrophysics And Space Physics (in Russian) (Nauka, M., 1982) p. 12
Friedman J L, J R Ipser, and L Parker Astrophys. 304 115 (1986)
Lang K R Astrophysical Formulae: A Compendium For The Physicist And Astrophysicist (Mir., M., 1978)
Alpar M A, M A Ruderman, and J Shaham Nature 300 728 (1982)
Taylor J H an D R Stinebring Ann. Rev. Astron. Astrophys. 24 285 (1986)
Kato M Publ. Astr. Soc. Jpn. 35 33 (1983)
Quinn T and B Paczynski Astrophys. 289 634 (1985)
Ebisuzaki T and K Nomoto Astrophys. 305 L67 (1986)