Точные решения уравнений Эйнщтейна - Крамер Д.
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King, A. R., and Ellis, G. F. R. (1973). Tilted homogeneous cosmological models, Commun. Math-Phys. 81, 20». See § 12.1.
Kinnersley, W. (1969a). Field of an arbitrarily accelerating point mass, Phys. Rev 186 1336. See §§ 28.1., 28.4.
Kinnersley, W. (1969b). Type D vacuum metrics, J. Math. Phys. 10, 1195. See S§7.1.. 11 3„
19.1., 24.1., 25.5., 27.5., 31.3.
Kinnersley, W. (1973). Generation of stationary Einstein-Maxwell fields, J. Math. Phys. 14. 651. See § 30.3.
Kinnersley, W. (1975). Recent progress in exact solutions, in: Shaviv, G., and Rosen, J. (Ed.). General Relativity and Gravitation (Proceedings of GR7, Tel-Aviv 1974), Wiley, New York, London. See §§ 1.1., 1.4., 11.3., 24.1., 30.3.
Kinnersley, W. (1977). Symmetries of the stationary Einstein-MaieweU field equations. I, J. Math. Phys. 18, 1529. See § 30.4.
Kinnersley, W. See also Walker and Kinnersley (1972)
Kinnersley, W., and Chitre, D. M. (1977— 78). Symmetries Ы Ihe'-etationary Einstein- Maxwelt field equations. 11—IV, J. Math. Phys. 18, 1538; 19, 1926, 2037. See § 30.4.
Kinnersley, W., and Chitre, D. M. (1978). Group transformation that generates the Kert and Tomimatsu-Sato metrics, Phys. Rev. Lett. 40, 1608. See §§ 30.4., 30.5.
Kinnersley, W., and Kelley, E. F. (1974). Limits of the Tomimatsu-Sato gravitational field. J. Math. Phys. 15, 2121. See § 18.6.
Kinnersley, W., and Walker, M. (1970). Uniformly accelerating charged mass in general relativity, Phys. Rev. D 2, 1359. See §§ 19.1., 28,1.
Kitamura, S. See Ikeda et al. (1963), Takeno and Kitamura (1968, 1969)
Klein, O. (1947). On a case of radiation equilibrium in general 'relativity theory and its bearing on the early stage of stellar evolution. Ark. Mat. Astr. Fys. A 84, 'I. See § 14.1.
Klein, 0. (1953). On a class ol spherically symmetric solutions of Einstein's gravitational equations, Ark. Fys. 7, 487. See § 14.1.
Klekowska, J., and Osinovsky, М. E. (1973). Group-theoretical analysis of some type Л' solution* of the Einstein field equations in vacuo, Preprint ITP-73-II7E, Kiev. See § 10.2.
Knight, W-R., and Bergraann, 0. <1974). Interacting matter and radiation in homogeneous isotropic worbl models. Int. J. Theor. Phys. 9, 47. See § 12.2.
Kobayashi, S., and Nomizu, K. (1969). Foundations of Differential Geometry (2 vols.) Inter-science Tracts in Pure and Applied Mathematics, 15, Interscience, Ne» York See § 2.1.
Kobiske, R. A., and Parker, L. (1974). Solution of the Einstein-Maxwell equations fat hro unequal spinning sources in equilibrium, Phys. Rev. D 10, 2321. See § 19.1.
Kohler, M., and Chao, K. L. (1965). Zentralsymmetrische statische Schwerefelder mil Raumen der Klasse I, Z. Naturforsch. 20a, 1537. See § 32.4.
Kohler, E., and Walker, M. (1975). A remark on the generalized Goldberg-Saihs theorem. GRG 6. 507. See §22.1.
Komar, A. B. See Bergmann et al. (1965)
Kompaneete, A. S. (1958). Strong gravitational waves in vacuum (in Bussian), Zh. Eksper. Teor. Fiz. 84, 953. See § 20.3.
Kompaneets,-A. S. (1959). Propagation of a strong electromagnetic-gravitational wave in vacuum (in Russian), Zh. Eksper. Teor. Fiz. 37, 1722. See § 20.4.
Kompaneete, A. S., and Chernov, A. S. (1964). Solution of the gravitation equations for a homo-уелеоия anisotropic model (in Russian), Zh. Eksper. Teor. Fiz. 47, 1939. See § 12.3.
ivota, J., and Perj6e, Z. (1972). AU stationary vacuum metrics with shearing geodesic eigenrays. J. Math. Phys. 18, 1695. See § 16.5.
Kottlor, F. (1918). Ober die physikalischen Qrundlagen der Einsteinschen Gravitationstheorie. Annalen Physik 56, 410. See § 13.4.
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Kowalczynski, J. К. (1978). Charged tachyon in general relativity. can it be delected?, Phys. Letters A 66, 269. See § 24.2.
Kowalczyiiski, J. K., nnd Plebanski, J. F. (1977). Jfelric and Jticci tensors for a certain class of «pace-times of D type. Int. J. Thcor. Phys. 16, 371. See § 27.7.
Kozarzewski, B. (1965). Asymptotic properties of the electromagnetic and gravitational fields, Acta Phys. Polon. 27, 775. See § 22.1.
Kramer, D. (1972). Gravitational field of a rotating radiating source, Third Sov. Grav. Conf. Erevan. Tezisj-, 321. See § 26.6.
Kramer, D. (1977). Einstein-Maxvxll fields with null Killing vector, Acta Phys. Hung. 48, 125. See § 30.5.
Kramer, D. See also Xeugebauer and Kramer (1969)
Kramer, D., and Neugebauer, G. (1968a). Algebraisch speziellt Minstein-Saume mit tiner Bewegungsgruppe, Commun. Math. Phys. 7, 173. See § 27.5.
Kramer, D., and Neugebauer, G. (1968b). Zu axialsymmetrischen stationaren Losungen der-Einsteinschen Feldgleiehungen fur das Vakuum, Commun. Math. Phys. 10, 132. See §§ 17.5.,
30.4.
Kramer, D., and Neugebauer, G. (1969). Eine exakte stationdre Losung der Einstein-MaxweU-Gleichungen, Annalen Physik 24, 59. See § 30.5.
Kramer, D., and Neugebauer, G. (1971). Innere Jieissner-Weyl-Losung, Annalen Physik 27, 129. See § 30.5.
Kramer, D., Neugebauer, G., and Stephani, H. (1972). Konstruktion und Charalterisiervnf von Oravitat ionsfeldem, Fortschr. Phyeik 20, I. See §§30.3., 30.5., 32.4.
