Рівняння Толмена — Опенгеймера — Волкова (Ukrainian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Рівняння Толмена — Опенгеймера — Волкова" in Ukrainian language version.

refsWebsite

Global rank Ukrainian rank

8harvard.edu

18^th place

74^th place

7doi.org

2^nd place

4^th place

4arxiv.org

69^th place

188^th place

4nih.gov

4^th place

5^th place

2archive.org

6^th place

2caltech.edu

887^th place

1,242^nd place

1goethe-university-frankfurt.de

low place

archive.org (Global: 6^th place; Ukrainian: 6^th place)

Oppenheimer, J. R.; Volkoff, G. M. (1939). On Massive Neutron Cores. Physical Review. 55 (4): 374—381. Bibcode:1939PhRv...55..374O. doi:10.1103/PhysRev.55.374.
Bombaci, I. (1996). The Maximum Mass of a Neutron Star. Astronomy and Astrophysics. 305: 871—877. Bibcode:1996A&A...305..871B.

arxiv.org (Global: 69^th place; Ukrainian: 188^th place)

Margalit, B.; Metzger, B. D. (1 грудня 2017). Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817. The Astrophysical Journal. 850 (2): L19. arXiv:1710.05938. Bibcode:2017ApJ...850L..19M. doi:10.3847/2041-8213/aa991c.
Shibata, M.; Fujibayashi, S.; Hotokezaka, K.; Kiuchi, K.; Kyutoku, K.; Sekiguchi, Y.; Tanaka, M. (22 грудня 2017). Modeling GW170817 based on numerical relativity and its implications. Physical Review D. 96 (12): 123012. arXiv:1710.07579. Bibcode:2017PhRvD..96l3012S. doi:10.1103/PhysRevD.96.123012.
Ruiz, M.; Shapiro, S. L.; Tsokaros, A. (11 січня 2018). GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass. Physical Review D. 97 (2): 021501. arXiv:1711.00473. Bibcode:2018PhRvD..97b1501R. doi:10.1103/PhysRevD.97.021501. PMC 6036631. PMID 30003183.
Rezzolla, L.; Most, E. R.; Weih, L. R. (9 січня 2018). Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars. Astrophysical Journal. 852 (2): L25. arXiv:1711.00314. Bibcode:2018ApJ...852L..25R. doi:10.3847/2041-8213/aaa401.

caltech.edu (Global: 887^th place; Ukrainian: 1,242^nd place)

authors.library.caltech.edu

Tolman, R. C. (1934). Effect of Inhomogeneity on Cosmological Models (PDF). Proceedings of the National Academy of Sciences. 20 (3): 169—176. Bibcode:1934PNAS...20..169T. doi:10.1073/pnas.20.3.169. PMC 1076370. PMID 16587869.
Tolman, R. C. (1939). Static Solutions of Einstein's Field Equations for Spheres of Fluid (PDF). Physical Review. 55 (4): 364—373. Bibcode:1939PhRv...55..364T. doi:10.1103/PhysRev.55.364.

doi.org (Global: 2^nd place; Ukrainian: 4^th place)

Oppenheimer, J. R.; Volkoff, G. M. (1939). On Massive Neutron Cores. Physical Review. 55 (4): 374—381. Bibcode:1939PhRv...55..374O. doi:10.1103/PhysRev.55.374.
Tolman, R. C. (1934). Effect of Inhomogeneity on Cosmological Models (PDF). Proceedings of the National Academy of Sciences. 20 (3): 169—176. Bibcode:1934PNAS...20..169T. doi:10.1073/pnas.20.3.169. PMC 1076370. PMID 16587869.
Tolman, R. C. (1939). Static Solutions of Einstein's Field Equations for Spheres of Fluid (PDF). Physical Review. 55 (4): 364—373. Bibcode:1939PhRv...55..364T. doi:10.1103/PhysRev.55.364.
Margalit, B.; Metzger, B. D. (1 грудня 2017). Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817. The Astrophysical Journal. 850 (2): L19. arXiv:1710.05938. Bibcode:2017ApJ...850L..19M. doi:10.3847/2041-8213/aa991c.
Shibata, M.; Fujibayashi, S.; Hotokezaka, K.; Kiuchi, K.; Kyutoku, K.; Sekiguchi, Y.; Tanaka, M. (22 грудня 2017). Modeling GW170817 based on numerical relativity and its implications. Physical Review D. 96 (12): 123012. arXiv:1710.07579. Bibcode:2017PhRvD..96l3012S. doi:10.1103/PhysRevD.96.123012.
Ruiz, M.; Shapiro, S. L.; Tsokaros, A. (11 січня 2018). GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass. Physical Review D. 97 (2): 021501. arXiv:1711.00473. Bibcode:2018PhRvD..97b1501R. doi:10.1103/PhysRevD.97.021501. PMC 6036631. PMID 30003183.
Rezzolla, L.; Most, E. R.; Weih, L. R. (9 січня 2018). Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars. Astrophysical Journal. 852 (2): L25. arXiv:1711.00314. Bibcode:2018ApJ...852L..25R. doi:10.3847/2041-8213/aaa401.

goethe-university-frankfurt.de (Global: low place; Ukrainian: low place)

How massive can neutron star be?. Goethe University Frankfurt. 15 січня 2018. Процитовано 19 лютого 2018.

harvard.edu (Global: 18^th place; Ukrainian: 74^th place)

ui.adsabs.harvard.edu

Oppenheimer, J. R.; Volkoff, G. M. (1939). On Massive Neutron Cores. Physical Review. 55 (4): 374—381. Bibcode:1939PhRv...55..374O. doi:10.1103/PhysRev.55.374.
Tolman, R. C. (1934). Effect of Inhomogeneity on Cosmological Models (PDF). Proceedings of the National Academy of Sciences. 20 (3): 169—176. Bibcode:1934PNAS...20..169T. doi:10.1073/pnas.20.3.169. PMC 1076370. PMID 16587869.
Tolman, R. C. (1939). Static Solutions of Einstein's Field Equations for Spheres of Fluid (PDF). Physical Review. 55 (4): 364—373. Bibcode:1939PhRv...55..364T. doi:10.1103/PhysRev.55.364.
Margalit, B.; Metzger, B. D. (1 грудня 2017). Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817. The Astrophysical Journal. 850 (2): L19. arXiv:1710.05938. Bibcode:2017ApJ...850L..19M. doi:10.3847/2041-8213/aa991c.
Shibata, M.; Fujibayashi, S.; Hotokezaka, K.; Kiuchi, K.; Kyutoku, K.; Sekiguchi, Y.; Tanaka, M. (22 грудня 2017). Modeling GW170817 based on numerical relativity and its implications. Physical Review D. 96 (12): 123012. arXiv:1710.07579. Bibcode:2017PhRvD..96l3012S. doi:10.1103/PhysRevD.96.123012.
Ruiz, M.; Shapiro, S. L.; Tsokaros, A. (11 січня 2018). GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass. Physical Review D. 97 (2): 021501. arXiv:1711.00473. Bibcode:2018PhRvD..97b1501R. doi:10.1103/PhysRevD.97.021501. PMC 6036631. PMID 30003183.
Rezzolla, L.; Most, E. R.; Weih, L. R. (9 січня 2018). Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars. Astrophysical Journal. 852 (2): L25. arXiv:1711.00314. Bibcode:2018ApJ...852L..25R. doi:10.3847/2041-8213/aaa401.
Bombaci, I. (1996). The Maximum Mass of a Neutron Star. Astronomy and Astrophysics. 305: 871—877. Bibcode:1996A&A...305..871B.

nih.gov (Global: 4^th place; Ukrainian: 5^th place)

ncbi.nlm.nih.gov

Tolman, R. C. (1934). Effect of Inhomogeneity on Cosmological Models (PDF). Proceedings of the National Academy of Sciences. 20 (3): 169—176. Bibcode:1934PNAS...20..169T. doi:10.1073/pnas.20.3.169. PMC 1076370. PMID 16587869.
Ruiz, M.; Shapiro, S. L.; Tsokaros, A. (11 січня 2018). GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass. Physical Review D. 97 (2): 021501. arXiv:1711.00473. Bibcode:2018PhRvD..97b1501R. doi:10.1103/PhysRevD.97.021501. PMC 6036631. PMID 30003183.

pubmed.ncbi.nlm.nih.gov

Tolman, R. C. (1934). Effect of Inhomogeneity on Cosmological Models (PDF). Proceedings of the National Academy of Sciences. 20 (3): 169—176. Bibcode:1934PNAS...20..169T. doi:10.1073/pnas.20.3.169. PMC 1076370. PMID 16587869.
Ruiz, M.; Shapiro, S. L.; Tsokaros, A. (11 січня 2018). GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass. Physical Review D. 97 (2): 021501. arXiv:1711.00473. Bibcode:2018PhRvD..97b1501R. doi:10.1103/PhysRevD.97.021501. PMC 6036631. PMID 30003183.

Рівняння Толмена — Опенгеймера — Волкова (Ukrainian Wikipedia)

archive.org (Global: 6th place; Ukrainian: 6th place)

arxiv.org (Global: 69th place; Ukrainian: 188th place)

caltech.edu (Global: 887th place; Ukrainian: 1,242nd place)