Точные решения уравнений Эйнщтейна - Крамер Д.
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Cahen, M. (1964). On a class of homogeneous spaces in general relativity. Bull. Acad. Roy.
Belgique Cl. Sci- 60, 972. See § 10.5.
Cahen. M. See also Bergmann ct al. (1965), Debever and Cnhen (1960, 1961)
Cahen, M., and Debevcr, R. (1965). Sur Ie Ihiorime de Birkhoff, O.K. Acad. Sci. (Paris) 260. 815. See § 13.4.
Cahen, M., and Defrise, L. (1968). Lorentzian 4-dimensional manifolds with “local isotropy”.
Commun. Math. Phys. 11, 56. See. §§9.2., 10.3., 11.1., 11.3.
Cahen, M., and Leroy, J- (1965). Ondes gravitationnelles en presence d'un champ Hectromagni-tique, Bull. Acad. Roy. Belgique Cl. Sci. SI, 996. See §§ 22.1., 27.7.
Ca lion, M.. and Leroy, J. (1966). Exact solutions of Einstein-Maxwell equations, J. Math. Mech.
16, 501. See §§ 22.1., 27.7., 32.5.
Cahen, M., and McLenaghan, R. (!. (1968). Mitriques des espaces lorenlziens symitriquet, a quatre dimensions, C.R. Acad. Sci. (Paris) Л 266, 1125- See § 31.2.
Cahen, M., and Sengier, J. (1967). Espaces de dasse D admettant un champ ilectromagnitique^ Bull. Acad. Roy- Belgique Cl. Sci. 68, 801. See §24.2.
Cahen, M., and Spelkens, J. (1967). Espaces tie type III solutions des iquations de Maxu-ell-
Einstein, Bull. Acad. Roy. Belgique Cl. Sci. 53, 817. See §§ 22.1. 27.5.
Cahen. M., Debever, R., and Defrise, L. (1967). .4 complex rectorial fornmlism in general relativity, J. Math. Mecli. 16. 761. See §3.5.
Campbell, S. J.. and Wninwright, J. (1977). Algebraic computing and the Newman-Penrose forinalism in general relativity, (!RO 8, 987. See § 7.1.
Captan, T. A. See Dnvies and Caplnn (1971)
Caporali. A. (1978). Non-existence for stationary, axially symmetric, asymptotically flat solutions of the Einstein equations for dust, Phys. Loiters A 66, 5. See § 19.2.
Carlson, G. T., and Snfko, J. L. (1978). An investigation of some of the kinematical aspects of
plane symmetric space-times, J. Math. Phys. 19. 1617. See § 13.4.
Carmeli, M. (1977V Group Theory and General Relativity, McGraw-Hill, New York. p. 244. See § 22.3.
Carter, B. (1968a). Hamilton-Jacobi and Schriklinger separable solutions of Einstein's equation».
Commun. Math. Phys. 10. 280. See § 19.1.
Carter. B. (1968b). А пеціатіїу ol Einstein spaces. Phys. Letters A 26. 399. See §§ 13.4.. 18.5.,
19.1.. 25.5., 27.5.
Carter. B. (1970). The commutation property ot a stationary, axisymmetric system. Commun.
Math. Phys 17. 233 See § 17 I.
Carter. B (1972). Black hole equilibrium sUtles,in: DeWitt, B., and D. (Eds.), Black Holes (Lee Hottchee'Leotiires 1972), Gordon and Breach. New York. See §§ 16.4., 17.2.. 18.5.. 19.1. Case. L A (1968) Changes of the Petrov type of a space-time, Phys. Rev. 176, 1554. See § 4.2-
378
CJhaTfravarty, N., Dutta Choudhoury, S. B.. and Banerjee, A. (1976). NoiMtatic spherically symmetric solutions for a perfect fluid in general relativity. Austral. J. Phys. 29, 113. See § 14.2. Chandrasekhar, S. (1978). The Kerr metric and stationary axisymmetric gravitational field*.
Proc. Roy. Soc. Lond. A 858, 405. See §§ 17.5., 18.5.
Chao, K. L. See Kohler and Ch.io (1965)
Chazy, J. (1924). Sur la champ de gravitation de deux masses fixes dans la theorie de la relallvite, Bull. Soc. Math. France 52, 17. See § 18.1.
Chernov, A. S. See Kompaneets and Chernov (1964)
Chinnapared, K. See Newinan et al. (1965)
Chitre, D. M. See Kinneralcy and Chitre (1977 — 1978, 1978)
Chitre, D. M., Giiven, R., and Xutku1 Y. (197.Ї). Static cylindrical!;/ symmetric solutions of the Einsttin-Maxwell equations, J. Math. Phys. 16, 475. See § 20.2.
Churchill, R. V. (1932). Canonical forms for symmetric linear vector functions in pseudo-eucl'itan space, Trans. Amer. Math. Sле. 34, 784. See § 5.1.
Clark, R. S. See Brickell and Clark (1970)
Clarke, C. J. (1970). On the isometric global embedding of pseudo-Riemannian manifolds. Proc.
Roy. Soc. Lond. A 814, 417. See § 32.7.
Cohen, J. M. See Batakis and Cohen (1972)
V.bhn, P. M. (1957). Lie Groups, Cambridge Univ. Press. See § 8.1.
Coll, B. (1975,4). Sur I'invariance du champ electromagnetique dans un espace-temps d'Einstein-Maxwell admetlant un groupe d'isometrie». C.R. Acad. Усі. (Paris) A 280, 1773. See § 9.1.
Coll. B. (197.>b). Sur la determination, par des donnies de Cauchy des champs de Killing ad mis par un espace-temps d’Einstein-MaxweU. (.'.R. Acad. Sci. (Paris) A 281, 1109. See §31.4. Collins, С. B. (1971). More qualitative cosmology. Commun. Math. Phye. 23, 137. See §§ 11.2..
11.3., 12.3., 12.4.
Collins, С. B. (1972). Qualitative magnetic cosmMogy, Commun. Math. Phys. 27.37. See §§ 11.3..
12.4.
Collins, С. B. (1974). Tilting at cosmological singularities. Commun. Math. Phys. 39, 131. See §§ 11.4., 12.3.
Collins, С. В. (X977). Global structure of the ‘ Kantowski-Sachs’ cosmological models, J. Math.
Phys. 18, 2116. See §§8.2., 11.1., 12.3., 13.1.
Collins, C. B., Glass, E. N.. and Wilkinson. D. (1980). Exact homogeneous rosmologies, GRG (to appear). See § 12.3.
