Точные решения уравнений Эйнщтейна - Крамер Д.
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Collinson, C. D. (1964). Symmetry properties of Harrison space-times. Proc. Camb. Phil. Soc. 60, 259. See § 15.4.
Collinson, C. D.(1966). Empty space-times of embedding class two, J. Math. Phys. 7,608. See § 32.5. Collineon, C. D. (1967). Empty space-times algebraically special on a given world line or hyper-surface, J. Math. Phys. 8, 1547. See § 7.5.
Collineon, C. D. (1968a). Embedding of the plane-fronted uxives and other space-times. J. Math.
Phys. 9, 403. See §§ 32.1., 32.5., 32.6.
Collinson, C. D. (1968b). Eimtein-Maxwell fields of embedding class one. Commnn. Math. Phys. 8, I. See § 32.4.
Collinson, C. D. (1969). Symmetries of type N empty space-times possessing twisting geodesic rays, J. Phys. A 2, 621. See § 33.2,
Collinson, C. D. (1970). Curvature' collineationx in empty space-times, J. Math. Phys. 11. 818. See §31.4.
Collinson, C. D. (1974). The existence of Killing tensors in empty space-times. Tensor 2S, 173. See § 31.3.
Collinson, C. D. (1976a). The uniqueness of the Schtearzschild interior metric. O.RG 7. 419. See § 19.2.
Collinson, C. D. (1976b). On the relationship between Killing tensors and Killing-Yano tensors.
Int. J. Theor. Phys. 15, 311. See § 31.3.
Collinson, C. D., and Dodd, R. K. (1969). Petrov classification of stationary axisymmetric
empty space time, N. Cim. B 62. 229. Set § 17.5.
Collinson, C. D., and Dodd, R. K. (1971). Symmetries of stationary axisymmetric empty space times, N. Cim. B 3, 281. Set § 33.2.
Collinson. C. D.. and French, D. C. (1967). Null tttrad approach to motions in empty ipnre time, J. Math. Phys. 8. 701. See §§ 22.3. 24.1., 33.2.
Collinson, C. D., and Fugfcre, J. (1977). Empty space-times with separable Hamilton-Jacohi
equation. J. Phys. A 10. 745. See §31.3.
Collinson, С. І>., and Shaw, В. (X972). The Rainich conditions for neutrino fields. Int. J. Theor. Phys. в, 347. See § 5.1.
Cook, M. W. (1975). On a does of exact spherically symmetric solutions to the Einstein gravitational field equations, Austral. J. Phys. 28, 413. See § 14.2.
Cosgrove, С. M. (1977). New family of exact stationary axisymmetric gravitational fields generalising the Tomimatsu-Salo solutions, J. Phys. A10, 1481. See § 18.6.
Cosgrove, С. M. (1978). A new formulation of the field equations for the stationary axisymmetric vacuum gravitational field, I. GeneroJ theory, II, Separable solutions, J. Phys. A11.2389.2405. See Il 18.6., 31.3.
Couch, E. See Newman et al. (1965)
Cox, D., and Flaherty, E. J. (1976). A conventional proof of Kerr's theorem, Commun. .Math.
Phys. 47, 75. See § 28.1.
Ourzon, H. E. J. (1924). Cylindrical solutions of Einstein's gravitation equations. Proc. London Math. Soc. 28, 477. See § 18.1.
Sale, P. (1978). Axisymmfitric gravitational fields: a nonlinear differential equation that admits a series of exact eigenfunction solutions, Proc. Boy. Soc. Lond. Л 362, 463. See § 18.6. DamiSo Sonres, I., and Assad, M. J. D. (1978). Anisotropic Bianchi \lllflX cosmological models with matter and electromagnetic fields, Phys. Letters A 66, 359. See § 12.3.
Darmois, G. (1927). Les Equations de la gravitation einsteiniennt, Memorbil rtos .«cirnces mnth?-matique, Fasc. XXV, Gauthier-Villnrs, Paris. See § 18.1.
Das, A. (1973). Static gravitational fields. II, Ricci rotation coefficients, J. Math. Phys. 14, 1099. See § 16.6.
Das, A. See also Zenk and Das (1978;
Das, К. C., and Banerji, S. (1978). Axially symmetric stationary solutions of Einstein-Maxwell equation!, GBG 9, 845. See § 30.5.
Datt, B. (1938). Ober eine Klasse ton Losungen tier Gravitationsgleichungen der Relativitat, Z. Phys. 108, 314. See § 13.5.
Datta, В. K. (1965). Homogeneous nonstatic electromagnetic fields in general relativity, X. Cira.
36, 109. See § 11.3.
Datta, В. K. (1967). Nonstatic electromagnetic fields in general relativity, N. Cim. A 47, 568. See § 13.4.
Dautcourt, G. (1964). Gravitationsfelder mit isotropem Killingveitor, in: Infeld, L. (Ed.), Relativists-Theories of Gravitation, Pergamon Press, Gauthier-Villars, PWN, p. 300. «See §21.4. Davies, H., and Caplan, T. A. (1971). The space-time metric inside a rotating cylinder, Proc.
Camb. Phil. Soc. 68, 325. See § 20.2.
Davis, Т. M. (1976). A simple application of the Newman-Penrose spin coefficient formalism.
I and 11, Int. J. Theor. Phys. 15, 315 (I), 15, 319 (II). See §7.1.
Davis, W. R. See Katzin efal. (1969)
Davis, W. R., Green, L. H., and Norris, L. K. (1976). Relativistic matter fields admitting Ricci collineations and related conservation laws, N. Cim. B 84, 256. See § 31.4.
De, U. K., and Banerjee, A. (1972). Two classes of solutions of null electromagnetic radiation. Prog. Theor; Phys. 47, 1204. See § 21.4.
Debever. R. (1959). Tenseur de avper-inergie, tenseur de Riemann: cas singuliers. C-R. Acad.
Sci. (Paris) 249, 1744. See l 4.3.
Debever, R. (1960). Espaces-temps du type III de Petrov, C.R. Acad. Sci. (Paris) 251. 1352. See § 27.5.
