Фейнмановские лекции по гравитации
Шрифт:
[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
[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-Nordstr"om 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.
[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. G"ottingen, 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.