ნეიტრონული ვარსკვლავი (Georgian Wikipedia)

Analysis of information sources in references of the Wikipedia article "ნეიტრონული ვარსკვლავი" in Georgian language version.

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  • Hessels, Jason; Ransom, Scott M.; Stairs, Ingrid H.; Freire, Paulo C. C.; et al. (2006). „A Radio Pulsar Spinning at 716 Hz“. Science. 311 (5769): 1901–1904. arXiv:astro-ph/0601337. Bibcode:2006Sci...311.1901H. doi:10.1126/science.1123430. PMID 16410486.
  • Hessels, Jason W. T; Ransom, Scott M; Stairs, Ingrid H; Freire, Paulo C. C; Kaspi, Victoria M; Camilo, Fernando (2006). „A Radio Pulsar Spinning at 716 Hz“. Science. 311 (5769): 1901–1904. arXiv:astro-ph/0601337. Bibcode:2006Sci...311.1901H. CiteSeerX 10.1.1.257.5174. doi:10.1126/science.1123430. PMID 16410486.
  • Abbott, B. P.; et al. (LIGO Scientific Collaboration & Virgo Collaboration) (16 October 2017). „GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral“. Physical Review Letters. 119 (16): 161101. arXiv:1710.05832. Bibcode:2017PhRvL.119p1101A. doi:10.1103/PhysRevLett.119.161101. PMID 29099225.
  • Demorest, Paul B.; Pennucci, T.; Ransom, S. M.; Roberts, M. S.; Hessels, J. W. (2010). „A two-solar-mass neutron star measured using Shapiro delay“. Nature. 467 (7319): 1081–1083. arXiv:1010.5788. Bibcode:2010Natur.467.1081D. doi:10.1038/nature09466. PMID 20981094.
  • Antoniadis, John (2012). „A Massive Pulsar in a Compact Relativistic Binary“. Science. 340 (6131): 1233232. arXiv:1304.6875. Bibcode:2013Sci...340..448A. CiteSeerX 10.1.1.769.4180. doi:10.1126/science.1233232. PMID 23620056.

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  • Pavlov, George; Zavlin, Slava; Sanwal, Divas; Kargaltsev, Oleg; Romani, Roger. Thermal Radiation from Isolated Neutron Stars. SLAC National Accelerator Laboratory. ციტირების თარიღი: 28 April 2016.

tempolimit-lichtgeschwindigkeit.de

  • Zahn, Corvin. (1990-10-09) Tempolimit Lichtgeschwindigkeit German. ციტატა: „Durch die gravitative Lichtablenkung ist mehr als die Hälfte der Oberfläche sichtbar. Masse des Neutronensterns: 1, Radius des Neutronensterns: 4, ... dimensionslosen Einheiten (c, G = 1)“ ციტირების თარიღი: 2009-10-09.

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scienceworld.wolfram.com

  • Magnetic energy density for a field B is U = B2/2μ0 per Eric Weisstein's World of Physics. Substituting B = 108 T, U = 4×1021 J/m3. Dividing by c2 one obtains the equivalent mass density of 44500 kg/m3, which exceeds the standard temperature and pressure density of all known materials, cf. 22590 kg/m3 for osmium, the densest stable element.

worldcat.org