Точные решения уравнений Эйнщтейна - Крамер Д.
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Israel, W. (1970). Differential forms in general relativity, Commun, Dublin Inst. Adv. Stud. A19. See §§2.1., 3.4.
Israel, W., and Khan, K. A. (1964). Collinear particles and Bondi dipoles in general relativity, N. Cim. 38, 331. See § 18.1.
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Israel, W., and Spanos1 J. T. J. (1973). Equilibrium of charged spiiming masses in general relativity, N. Cim. Lett. 7, 245. Sec § 16.7.
Israel, W., and Wilson, G. A. (1972). -4 class of stationary electromagnetic vacuum fields, J. Math. Phys. 13, 865. See § 16.7.
Лее, VV. С. W. See Wainwright et al. (1979)
Jacobs, К. C. (1968). Spatially homogeneous and Euclidean cosmological models with shear, Astrophys. J. 153, 661. See §§ 12.3., 12.4.
Jacobs, К. C. (1969). Cosmologies of Bianchi type I with a uniform magnetic field, Astrophys. J. 156, 379. See §§ 11.3., 12.1., 12.4.
Jeffery, G. B. See Baldwin and Jeffery (1926) ,
Jordan, P., and Kundt, W. (1961). Geometrodynamik im Null fall, Akad. Wise. Lit. Mainz. Abhandl. Math.-Nat. Kl. 1961 no. 3. See § 5.4.
Jordan, P., Elilers, J., and Kundt, W. (1960). Strenge Ldsungen der Feldgleichungen der AU-gemeinen Relatimtatstheorie, Akad. Wiss. Lit. Mainz. Abliand)., Math.-Nat. Kl. 1960 no. 2. See §§ 3.4., 3.6., 3.7., 16.1., 21.5.
Jordan, P., Ehlers, J., and Sachs, R. K. (1961). Beitrage гиг Theorie der reinen Gravitations-strahlung, Akad. Wiss. Lit. Mainz, Abhandl. Math.-Nat. Kl. 1960 no. I. See §§ 4.3., 6.1.
Joseph, V. (1966). A spatially homogeneous gravitational field, Proc. Camb. Phil. Soc. 62, 87. See §11.3.
Kaigorodov, V. R. (1962). Einstein spaces of maximum mobility (in Russian), DokI. Akad. Nauk SSSR 146, 793. See §§ 10.5., 33.2.
Kaigorodov, V. R. (1967). Exact type III solutions of the field equations Rjj = 0 (in Russian),
Grav. і Teor. Otnos., Univ. Kazan 3, 155. See § 27.5.
Kaigorodov, V. R. (1972). Petrov classification and recurrent spaces (in Russian), Gravitatsiya, Nauk dumka, Kiev, 52. See § 31.2.
Kalnins, Ё. G. See Boyer et al. (1978)
Kammerer, J. B. (1966). Sur Ies directions principales du tenseur de courbure, C.R. Acad. Sci. (Paris) 263, 533. See § 7.4.
Kantowski, R. (1966). Some relativisiic cosmological models, Pb. D. Thesis, Univ. of Texas. Stt §§11.1., 12.3.
Kantowski, R., and Sachs, R. K. (1966). Some spatially homogeneous anisotropic relativisiic cosmological models, J. Math. Phys. 7, 443. See §§ 11.1., 12.3.
Ksrmarkar, K. R. (1948). Gravitational metrics of spherical symmetry and class one, Proc.
Indian Acad. Sci. Л 27, 56. See § 32.3.
Karmarkar, K. R. See also Narlikar and Karmarkat' (1946)
Kasner, E. (1921). Geometrical theorems on Einstein's cosmological equations, Amer. J. Math. 43, 217. See § 11.3.
Katz in. G. H,, and Levine, J. (1972). Applications of Lie derivatives to symmetries, geodesic mappings, and first integrals in Iliemannian spacts. Colloquium Math. 26, 21. See § 31.4.
Kat'/.in, (_!. H., Levine1J., and Davis, W. R. (1969). Curvature collineations: A fundamental symmetry property of the space-times of general relativity definedbythe vanishing Lie derivative of Ihe Riemann curvature tensor, J. Math. Phys. 10, 617. See § 31.4.
Kelley, E. F. See Kinnersley and Kelley (1974)
Kellner, A. (1975). I-dimensionale Gravitatiotisfelder, Dissertation Gottingen. See §§ 11.1., 11.3.
Kerr, R. P. (1963a). Gravitational field of a spinning mnss as an example of algebraically special metrics, Phys. Rev. Lett. 11, 237. See §§ 18.5., 25.1., 25.5.
Kerr1 R. P. (1963 b). Scalar invariants and groups of motions in a four dimensional Einstein space, J. Math. Mec-h. 12, 33. See §§ 8.4., 31.4.
Kerr, R. P. See also Debney et al. (1969), Farnsworth and Kerr (1966), Goldberg and Kerr (1961), Weir and Kerr (1977)
Kerr. R. P., and Debney, G. (1970). Einstein spaces with symmetry groups, J. Math. Phvs. II. 2807. See §§ 11.3., 25.2., 33.2.
Keri, R. P., and GoldberglJ. N. (1961). Einstein spacts with four-parameter holonomy groups, J. Math. Pbys. 2, 332. See § 27.5.
Kerr1 R. P., and Scbild, A. (1965). Some algebraically degenerate solutions of Einstein’s gravitational field equations, Proc. Symp. Appl. Math. 17, 199. See § 28.2.
Kerr, R. P., and Schild1 A. (1967). A new class of vacuum solutions of the Einstein field equations, in: Atti del convegno sulla relativita generale, Firenze, p. 222. See J 28.2.
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Khan, К. A. See Israel and Khan (1964)
Khan, K. A., and Penrose, R. (1971). Scattering of two impulsive gravitational ¦plane Uwetr Nature 22», 185. See § 15,2.
Kharbediya, L. I. (1976). Some exact solutions of the Friedmann equations with the cosmological term (in Russian)-, Astron. Zh. (USSR) 68, 1145. See § 12.2.
Khlebnikov, V. I. See Alekseev and Khlebnikov (1978), Frolov and Khlebnikov (1975) -•
King, A. R. (1974). New types of singularity in general relativity: the general cylindrically syw metric stationary dust solution, Commun. Math. Phys. 88, 157. See § 20.2.
.King, A. R. See also Ellis and King (1974)
