Точные решения уравнений Эйнщтейна - Крамер Д.
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Krasiiiski, A. (1975). Solutions of the Einstein field equations for a rotating perfect fluid. II. Properties of the flow-stationary and vortex-homogeneous solutions, Acta Phys. Polon. B 6, 223. See § 20.2.
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Krishna Rao, J. (1963). Type-N gravitational waves in non-empty space-time, Curr. Sci. 82, 350. See § 20.4.
Krishna Rao, J. (1964). Cylindrical waves in general relativity, Proc. Nat. liut. Sci. India A SO, 439. See § 20.4.
Krishna Rao, J. (1970). Cylindrically symmetric null fields in general relativity, Inditn J. Pure
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Kuchowiez, B. (1966). Some new solutions of the gravitational field equations, Dept. Radio-chemistry, Univ. of Warsaw, Preprint. See § 14.1.
Kuchowicz, Bi (1967). Exact formulae for a general relativisiic fluid sphere. Phys. Letters A 26, 419. See § 14.1.
Kuchowicz, B. (1968). General relativistic fluid spheres. I. New solutions for spherically sym-
metric matter distributions, Aota Phys. Polon. 88, 541. See § 14.1.
Kuchowicz, B. (1970). General ¦ relativistic fluid spheres. III. A simultaneous solving of two equations, Acta Phys. Polon. B I, 437. See § 14.1.
Kuchowicz, B. (1972). General relativistic fluid spheres. V. Norn-charged static spheres of perfect
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Kundt, W. (1961). The plane-fronted gravitational waves, Z. Phys. 163, 77. See SS 21 4 27 I
27.2., 27.5. 2 ’ '*
Kundt, W. (1962). Exact solutions of the field equations: twist-free pure radiation fields, Proc#
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Kundt, W. See also EMers and Kundt (1962), Jordan and Kundt (1961), Jordan et al. (1960)
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Kundt, VV., and Triimper, M. (1962). Beitrage гиг Theorie der Oravitations-Strahlungsfeldert Akad. Wise. Lit. Mainz, Abhandl. Math.-Nat. Ki. 1982 no. 12. See §§ 7.5., 21.4., 27.1., 29.4»
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389
Kustaanheimo, P. (1947). Some remarks concerning (he connexion between two spherically symmetric relativistic metrics, Comment. Phys. Hath., Helsingf. 18, 8. See § 14.2.
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ІЛІ, K. B., and Prasad, H. (1969). Cylindrical wave solutions of field equations of general relativity containing electromagnetic fields, Tensor 20, 45. See § 20.4.
Lanczos, C. (1962). The splitting'pf the Riemann tensor, Rev. Mod. Phys. 84,379. See §§ 3.5., 3.6.
Land, VV. J. See Buchdahl and Land (1968)
Lauten III, W. T., and Ray, J. R. (1975). Space-times with groups of motions on null hyper-surfaces, X. Cim. Lett. 14, 63. See § 21.2.
Lauten III, \V. T., and Ray, J. R. (1977). Investigations of space-times with four-parameter groups of motions acting on null hypersurfaces, J. Hath. Phys. 18, 885. See $ 21.2.
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Lemaitre, G. (1927). Un univers homogine it masse constants et de rayon croissant, rendant compte de la vitesse radiale de nebuleuses extra-galactiques, Ann. Soc. Sci. Bruxelles A 47, 49. See S 12.2.
Lemaitre, G. (1933). L'univers en expansion, Ann. Soc. Sci. Bruxelles I A 68, 61, See §§ 13.4., 13.5.
Leroy, J. (1970). Un espace d'Einstein de type. N d rayons non inUgraibles, C.R. Acad. Sci. (Paris) A 270,1078. See § 11.3.
Leroy, J. (1976). Champs Oectromagnitiques a rayons intigrablis, divergent» et sans distorsion, Bull. Acad. Roy. Belgique Cl. Sci. 62, 259. See § 24.2.
Leroy, J. (1978). Sur une classe d'espace e-temps solutions des equations d'Einstein-Maxu/ell, Bull. Acad. Roy. Belgique Cl. Sci. 64,130. See $ 26.5.
Leroy, J. See also Cahen and Leroy (1965,1966), HcLenaghan and Leroy (1972)
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