Фейнмановские лекции по гравитации

[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).

[Wald 86] Wald, Robert M. (1986). ”Spin-two fields and general covariance,” Physical Review, D33, 3613-3625.

[Wein 64a] Weinberg, Steven (1964). ”Derivation of gauge invariance and the equivalence principle from Lorentz invariance of the S-matrix,” Physics Letters, 9, 357-359.

[Wein 64b] Weinberg, Steven (1964). "Photons and gravitons in S-matrix theory: derivation of charge conservation and equality of gravitational and inertial mass,” Physical Review, 135, B1049-B1056.

[Wein 72] Weinberg, Steven (1972). Gravitation and Cosmology

(Wiley, New York). (Имеется русский перевод Вейнберг С. (1975) Гравитация и космология (Мир, Москва)).

[Wein 79] Weinberg, Steven (1979). ”Ultraviolet divergences in quantum theories of gravitation,” in General Relativity: An Einstein Centenary Volume, edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England), pp. 790-831. (Имеется руссхий перевод в сб.: Общая теория относительности, сс. 407-455, (Мир, Мосхва, 1983)).

[Wein 89] Weinberg, Steven (1989). ”The cosmological constant problem,” Reviews of Modem Physics, 61, 1-22.

[Went 49] Wentzel, G. (1949). Quantum Theory of Fields, (Interscience, New York).

[Whee 62] Wheeler, John A. (1962). Geometrodynamics, (Academic Press, New York).

[Whee 90] Wheeler, John A. (1990). A Journey into Gravity and Spacetime (Scientific American Library, W. H. Freeman, New York).

[WhFe 45] Wheeler, John A. and Feynman, Richard P. (1945). ”Interaction with the absorber as the mechanism of radiation,” Reviews of Modern Physics, 17, 157-181.