Фейнмановские лекции по гравитации

[Eddi 36] Eddington, A. (1936). Relativity Theory of Protons and Electrons (Cambridge University Press, Cambridge).

[Eddi 46] Eddington, A. (1946). Fundamental Theory (Cambridge University Press, Cambridge).

[Eins 39] Einstein, Albert (1939). ”On a stationary system with spherical symmetry consisting of many gravitating masses,” Annals of Mathematics, 40, 922-936.

[FaPo 67] Faddeev, L. D. and Popov, V. N. (1967). ”Feynman diagrams for the Yang-Mills Field,” Physics Letters B, 25, 29-30.

[Feyn 57] Feynman, Richard P. (1957). ”Conference on the Role of Gravitation in physics, an expanded version of the remarks by R. P. Feynman on the reality of gravitational waves, mentioned briefly on page 143 of the Report [DeWi 57],” typescript in Box 91, File 2 of The Papers of Richard P. Feynman, the Archives, California Institute of Technology.

[Feyn 61] Feynman, Richard P. (1961). Unpublished letter to Victor F. Weisskopf, January 4-February 11, 1961; in Box 3, File 8 of the Papers of Richard P. Feynman, the Archives, California Institute of Technology.

[Feyn 63a] Feynman, Richard P., Leighton, Robert B., and Sands, Matthew (1963). The Feynman Lectures on Physics (Addison-Wesley, Reading, Massachusetts) (Имеется русский перевод: Фейнман Р., Лейтон P., Сэндс М. (1965-1967) Фейнмановские лекции по физике, тт. 1-9 (Мир, Москва).

[Feyn 63b] Feynman, Richard P. (1963). ”Quantum theory of gravitation”,

Acta Physica Polonica, 24, 697-722.

[Feyn 67] Feynman, Richard P. (1967). The Character of Physical Law (M.I.T., Cambridge). (Имеется руссхий перевод: Фейнман P. (1968) Характер физических законов (Мир, Москва)).

[Feyn 72] Feynman, Richard P. (1972). ”Closed loop and tree diagrams” and ”Problems in quantizing the gravitational field, and the massless Yang-Mills field,” in Magic Without Magic: John Archibald Wheeler, edited by John R. Klauder (W.H. Freeman, San Francisco), pp. 355-408.

[Feyn 85] Feynman, Richard P., as told Leighton, Ralph (1985). Surely You’re Joking, Mr. Feynman! (W.W. Norton, New York).

[Feyn 88] Feynman, Richard P., as told Leighton, Ralph (1988). What Do You Care What Other People Think? (W.W. Norton, New York).

[Feyn 89] ”Feynman’s office: The last blackboards,” Physics Today, 42

(2), 88 (1989).

[FiPa 39] Fierz, M. and Pauli, W. (1939). ”Relativistic wave equations for particles of arbitrary spin in an electromagnetic field,” Proceedings of the Royal Society of London A, 173, 211-232.

[Fink 58] Finkelstein, David (1958). ”Past-future asymmetry of the gravitational field of a point particle,” Physical Review, 110, 965-967.

[Fowl 64] Fowler, William A, (1964). ”Massive stars, relativistic polytropes, and gravitational radiation,” Reviews of Modem Physics, 36, 545-555.

[FuWh 62] Fuller, Robert W. and Wheeler, John A. (1962). ”Causality and multiply connected space-time,” Physical Review, 128, 919-929.

[FWML 74] Fairbank, W., Witteborn, F., Madey, J., and Lockhart, J. (1974). ”Experiments to determine the force of gravity on single electrons and positrons,” Experimental Gravitation: Proceedings of the International School of Physics ”Enrico Fermi," Course LVI, B.Bertotti, ed. (Academic Press, New York) 310-330.

[Gell 89] Gell-Mann, Murray (1989). ”Dick Feynman-The guy in the office down the hall,”

Physics Today, 42 (2), 50-54.

[Good 61] Good, M.L. (1961). "K⁰₁ and the equivalence principle,” Physical Review, 121, 311-313.

[GoSa 86] Goroff, M. and Sagnotti, A. (1986). Nuclear Physics B, 266, 709.

[GrBr 60] Graves, John C. and Brill, Dieter R. (1960). "Oscillatory character of Reissner-Nordström metric for an ideal charged wormhole,” Physical Review

, 120,1507-1513.

[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.