Точные решения уравнений Эйнщтейна - Крамер Д.
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Debever, R. (1964). Le rayonnement grueitationnel: Le tenseur de Riemann en relntiviti ginentle, Cahiers Phys. 18, 303. See § 4.1.
Debever, R. (1965). Local tetrad in general relativity. In: Atti del convegno sulla relativita generate: problemi dell'energia e ondi gravitational!, Barbara, Firenze. See § 10.2.
Debever, R. (1966). Reprieentation vectorielle de la courbure en relativiti ginirale: transformations eonformes, in: Perspectives in Geometry and Relativity, Ind. Univ. Press, p. 96. See §§3.4., 3.7.
Debever, R. (1969). Sur Ies espaces de Brandon Carter, Bull. Acad. Roy. Belgique Cl. Sci. 55. 8. See § 19.1.
Debever, R. (1971). On type P expanding solutions of Einstein-Maxwtll equations. Bull. Soc.
Math. Belg. 23. 360. See §§ 19.1., 24.2., 25.5.
Debever, R. (1974). Sur une clause d'espaces lorentziens, Bull. Acad. Roy. Belgique Cl. Sci-60, Я98. See §28.1.
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Debever, R. (1976). Structures pre-maxwelliennes involutives en relativite g InltdXei Bull. Acad. Roy. Belgique Cl. Sci. 62, 662. See §§ 19.1., 26.5.
Debevcr, R. See also Cahen and Debever (1965), Cahen et al, (1967), G?h?niau and Debeyer (1956a, b)
Debever, R., and Cahen, M. (1960). Champs HectromagnMigues constants en relativite generate, C.R. Acad. Sci. (Paris) 251, 1160. See§ 31.1..
Debever, R., and Cahen, M. (1961). Sur Ies espaces-temps, gui admettent Ufi champ de vect6W3 isotropes par alleles, Bull. Acad. Roy. Belgique Cl. Sci. 47, 491. See §§ 6.1,, 6.2.
Debney, G. (1971). On vacuum space-times admitting a null Killing bivector. J. Math. Phys. 12, 2:ї72. See §§21.4., 27.5.
Debney, G. (1972a). Null Killing vectors in general relativity, N. Cim. Let*. 5, 954. See § 21.4.
Debney, G. (1972b). Symmetry in Einstein-Maxwell space-time, J. Hath. Phys. 18, 1469* See § 21.4.
Debney, G. (1973). Expansion-free Kerr-Schild fields, N. Cim. Lett. 8, 337. See §§ 27.6,, 28.2.
Debney, G. (1974). Expansion-free electromagnetic solutions of the Kerr-Schild class, J. Matb. Phys. 15, 992. See §§ 21.4., 27.6., 28.3.
Debney, G. See also Kerr and Debney (1970)
Debney, G., Kerr, R. P., and Schild, A. (1969). Solutions of the Einstein and Einsleln-Maxwell equations, J. Math. Phys. 10, 1842. See §§ 23.1., 25.1., 28.2., 28.3.
Defrise, L. (1969). Groupes d'isotropie et groupes de siabilite conforme dans Us espaces Iorentziensf These, Universite Libre de Bruxelles. See §§ 8.1., 8.4., 9.2., 10.1., 11.1.
Defrise, L. See also Cahen and Defrise (1968), Cahen et al. (1967)
Demianski, M. (1972). New Kerr-like space-time, Phys. Letters A 42, 157. See §§ 25.2., 30.C.
Demiariski, M. (1973). Some new solutions of the Einstein equations of astrophysical interestf Acta Astron. (Poland) 23, 197. See §§ 18.5., 30.6.
Demianski, M. (1976). Method of generating stationary Einsiein-Maxtcell fields, Acta PJays, Polon. B 7, 567. See § 30.3.
Demianski, M. See also Plebatiski and Demianski (1976}
Demianski, M., and Grishchuk, L. P. (1972). Homogeneous rotating universe with flat space, Commun.. Math. Phys. 25, 233. See § 12.4.
Demianski* M. and Newman. E. T. (1966). A combined Kerr-NXJT solution of the Einsteiiu field equations, Bull. Acad. Polon. Sci. Ser. Math. Astron, Phys, 14,653. See §§ 1'8.5.19.1./30,5.
de Sitter, W. See Einstein and de Sitter (1932)
Dietz, W. (1976). Separable coordinate systems for the Hamilton-Jacobi, Klein-Gordon and wave equations in curved spaces, J. Phys. A 9, 519. See § 31.3.
d’Inverno, R. A., and Russell-Clark, R. A. (1971). Classification of the Harrison metrics, «Г*
Math. Phys. 12, 1258. See §§ 4.4., 15.4.
Dodd, R. K. See Collinson and Dodd (1969, 1971)
Dolan, P. (1968). A singularity-free solution of the MaxwelLEinstein-equalion, Commun. jYtith. Phys. 9, 161. See §10.3.
Doroshkevich, A. G. (1965). Model of a universe with a uniform magnetic field (in Russian), Astrofiz. I, 255. See §§ 12.1., 12.3.
Dowker, J. S. See Roche and Dowker (1968)
Dozmorov, I. M. (1971). Solutions of the Eiiwiein equations related by null vectors. 77, III /in Russian). Izv. VUZ. Fiz. no. 11. 68 (II), no. 11, 76 (III). See § 28.5.
Dozmorov, I. M. (1973). The algebraic classification of the matter tensor (in Russian), Izv. VUZ. Fiz. no. 12, 101. See § 5.1.
buuu, K. A., and Tupper, B. 0. J. (1976)- A class of Bianchi type. VI cosmological models with electromagnetic field, Astrophys. J. 204, 322. See §§ 12.1., 12.4.
Dutta Choudhoury, S. B. See Chakravarty et al. (1976)
Eddington, A. S. (1924). A comparison, of Whitehead's and Einstein's formulae, Nature 113, 192. See § 13.4.
Edwards, D. (1972). Exact expressions for the properties of the zero-pressure Friedmann models, Mon. Not. Roy. Astr. Soc. 159, 51. See § 12.2.
Egorov, I. P. (1955). Riemannian spaces Vi of nonconstant curvature and maximum mobility (in Russian), Dokl. Akad. Nauk. SSSR 103, 9. See § 30.3.
Ehlers, J. (1957). Konstruktionen und Charakterisierungen von Losungen der Einsteinscien Gravitationsfeidgleichungen, Dissertation, Hamburg. See § 30.3.
