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[GSW 87] Green, М., Schwarz, J., and Witten, E. (1987). Superstring theory (Cambridge University Press, Cambridge, England).

[GrPe 88] Gross, D. and Periwal, V. (1988). ”String perturbation theory diverges,” Physical Review Letters, 60, 2105-2108.

[Gupt 54] Gupta, Suraj N. (1954). ”Gravitation and electromagnetism,” Physical Review, 96, 1683-1685.

[Guth 81] Guth, Alan H. (1981). ”Inflationary universe: a possible solution to the horizon and flatness problems,” Physical Review D, 23, 347-356.

[HaEl 73] Hawking, Stephen W. and Ellis, George F.W. (1973). The Large Scale Structure of Space-time, (Cambridge University Press, Cambridge, England). (Имеется русский перевод: Хокинг С., Эллис Дж. (1977) Структура пространства-времени (Мир, Москва)).

[Hatf 92] Hatfield, В. (1992). Quantum Field Theory of Point Particles and Strings, (Addison-Wesley, Reading, MA).

[Hilb 15] Hilbert, D. (1915). ”Die Grundlagen der Physik,” Konigl. Gesell. d.Wise. Göttingen, Nachhr. Math.-Phys. Kl., 395-407. (Имеется русский перевод в сб.: Альберт Эйнштейн и теория гравитации, (1979), с. 133—145 (Мир, Москва)).

[HoFo 63] Hoyle, Fred, and Fowler, William A. (1963). ”On the nature of strong radio sources,” Monthly Notices of the Royal Astronomical Society, 125, 169-176.

[Hoyl 48] Hoyle, Fred (1948). ”A new model for the expanding universe,” Mon. Not. R. Astron. Soc., 108, 372-382.

[HWWh 58] Harrison, B. Kent, Wakano, Masami, and Wheeler, John A. (1958). ”Matter-energy at high density; endpoint of thermonuclear evolution,” in Onzieme Conseil de Physique Solvay, La Structure et I’Evolution de I’Univers, (Editions R. Stoops, Brussels), pp. 124-148.

[Iben 63] Iben, Icko, Jr. (1963). ”Massive stars in quasistatic equilibrium,” Astrophysical Journal, 138, 1090-1096.

[JaSm 88] Jacobson, T. and Smolin, L. (1988). ”Nonperturbative quantum geometries,” Nuclear Physics B, 299, 295-345.

[JeDG 53] Jennison, R. C. and Das Gupta, М. K. (1953). ”Fine structure of the extra-terrestrial radio source Cygnus 1,” Nature, 172, 996-997.

[Klei 89] Kleinert, H. (1989). ”Quantum mechanics and path integrals in spaces with curvature and torsion," Modem Physics Letters A, 4, 2329-2337.

[Kore 74] Корепин, Владимир (1974). Неопубликованный диплом, Ленинградский Государственный Университет.

[Krai 47] Kraichnan, Robert H. (1947). ”Quantum theory of the linear gravitational field,” unpublished B.S. thesis, Massachusetts Institute of Technology.

[Krai 55] Kraichnan, Robert H. (1955). "Special relativistic derivation of generally covariant gravitation theory,” Physical Review, 98, 1118-1122.

[Krai 56] Kraichnan, Robert H. (1956). ”Possibility of unequal gravitational and inertial masses,” Physical Review, 101, 482-488.

[Krus 60] Kruskal, Martin (1960). "Maximal extension of the Schwarzschild metric,” Physical Review, 119, 1743-1745.

[LaLi 51] Landau, L .D. and Lifshitz, E. M. (1951). The Classical Theory of Fields, translated by M. Hammermesh (Addison-Wesley, Reading, Massachusetts) (Имеются оригинальные русские издания, например, Ландау Л.Д., Лифишц Е.М. (1988) Теория поля (Наука, Москва)).

[LiBr 90] Lightman, Alan and Brawer, Roberta (1990). Origins: The Lives and Worlds of Modem Cosmologists, (Harvard University Press, Cambridge).

[MaWh 66] May, Michael M. and White, Richard H. (1966). ”Hydrodynamical calculations of general relativistic collapse,” Physical Review, 141, 1232-1241.

[Mich 63] Michael, F. Curtis (1963). ”Collapse of massive stars,” Astrophysical Journal, 138, 1097-1103.

[Miln 34] Milne, E. (1934). Quart. J. Math (Oxford), 5, 64; McCrea, W. and Milne, E. (1934). Quart. J. Math (Oxford), 5, 73.

[MiWh 57] Misner, Charles W. and Wheeler, John A. (1957). ”Classical physics as geometry: gravitation, electromagnetism, unquantized charge, and mass as properties of curved empty space,” Annals of Physics, 2, 525-603 reprinted in [Whee 62].

[MTW 73] Misner, Charles W., Thorne, Kip S., and Wheeler, John A. (1973). Gravitation, (W.H. Freeman, San Francisco). (Имеется русский перевод Мизнер Ч., Торн К., Уилер Дж. (1977) Гравитация, тт. 1-3 (Мир, Москва)).

[NiGo 91] Nieto, М. and Goldman, Т. (1991). ”The arguments against ”antigravity” and the gravitational acceleration of antimatter,” Physics Reports, 205, 221-281.

[OpSn 39] Oppenheimer, J. Robert and Shyder, Hartland (1939). ”On Continued Gravitational Contraction," Physical Review, 56, 455-459. (Имеется руссхий перевод в сб.: Альберт Эйнштейн и теория гравитации, (1979), 353-361 (Мир, Москва)).

[Репг 65] Penrose, Roger (1965). ”Gravitational collapse and spacetime singularities,” Physical Review Letters, 14, 57-59. (Имеется русский перевод в сб.: Альберт Эйнштейн и теория гравитации, (1979), 390-395 (Мир, Москва)).

[Podu 64] Подурец М. А. (1964). ”Коллапс звезды с учётом противодавления,” Доклады Академии Наук, 154, 300-301.

[RoSm 88] Rovelli, С. and Smolin, L. (1988). ”Loop representation for quantum general relativity,” Nuclear Physics B, 331, 80-152.

[Schi 58] Schiff, L. (1958). ”Sign of the gravitational mass of the positron,” Physical Review Letters, 1, 254-255.

[Schi 59] Schiff, L. (1959). "Gravitational properties of antimatter,” Proc. Nat. Acad. Sci., 45, 69-80.

[Schm 63] Schmidt, Maarten A. (1963). ”3C 273: A star-like object with large red-shift,” Nature, 197, 254-255.

[Schu 85] Schutz, Bernard F. (1985). A First Course in General Relativity (Cambridge University Press, Cambridge).

[Schw 16] Schwazschild, Karl (1916). ”Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie,” Sitzungsberichte der Deutschen Akademie der Wissenschaften zu Berlinn, Klasse für Mathematik, Physik, und Technik, 1916, 189-196. (Имеется русский перевод в сб.: Альберт Эйнштейн и теория гравитации, (1979), 199-207 (Мир, Москва)).

[Syke 94] Sykes, Christopher (1994). No ordinary genius: the illustrated Richard Feynman (W. W. Norton, New York).

[Thir 18] Thirring, H. (1918). ”Über die Wirkung rotierender ferner Massen in der Einsteinschen Gravitationstheorie,” Phys. Z., 19, 33-39; Thirring, H. and Lense, J. (1918). ”Über den Einflufder Eigenrotation der Zentralkorper auf die Bewegung der Planeten und Monde nach der Einsteinschen Gravitationstheorie”, Phys. Z., 19, 156-163; Thirring, H. (1921). ”Berichtigung zu meiner Arbeit: ’Über die Wirkung rotierender ferner Massen in der Einsteinschen Gravitationstheorie’,” Phys. A., 22, 29-30.

[tHVe 74] t’Hooft, G. and Veltman, M. (1974). Ann. Inst. Henri Poincare, 20, 69.

[Thor 94] Thorne, Kip S. (1994). Black Holes and Time Warps: Einstein’s Outrageous Legacy, (W. W. Norton, New York).

[Toop 66] Tooper, Robert F. (1966). ”The’standard model’ for massive stars in general relativity,” Astrophysical Journal, 143, 465-482.

[vanN 81] van Nieuwenhuizen, Peter (1981). ”Supergravity,” Physics Reports, 68, 189-398.

[Vebl 27] Veblen, O. (1927). Invariants of Quadratic Differential Forms, (Cambridge Tracts in Math and Math Phys., Cambridge University Press, London). (Имеется руссхий перевод: Веблен О. (1948) Инварианты дифференциальных квадратичных форм (Гостехиздат, Москва)).

[Wald 84] Wald, Robert М. (1984). General Relativity, (University of Chicago Press, Chicago).

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