Точные решения уравнений Эйнщтейна - Крамер Д.
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Robinson. I., Schild, A., and Strauss, H. (1969b). A 'generalized Reissner-NoidetrOm solution. Int. J. Theor. Phys. 2, 243. See §§ 26.2., 26.3., 26.4.
Robinson, J. R. See Robinson and Robinson (1969), Robinson et «1. (1969 a)
Roche, J. A., and Dowker, J. S. (1968). The algebraic structure of the vacuum Riemam tensor, J. Phys. A I, 527. See § 4.2.
Roos, W. (1976). On the existence of interior solutions in general relativity, GRG 7,431. See {19.2. Roos1 W. (1977). The matter-vacuum matching problem in general relativity: general methods and special cases, GRG 8, 753. See § 19.2.
Bosen, G. (1962). Symmetries of the Einstein-Maxwell 'equations, J. Math. Phys. 8, 319, Am
S 11.3.
396
Rosen, J. (196"i). Embedding of various relativistic Riemannian spaces in pnetiilo-euclidean spaces, Rev. Mod. Phys. 37, 204. See §§ 32.1., 32.5.
Rosen, N. J. See Einstein and Rosen (1937)
Rosenblum, A. See Ehlers et al. (1976)
Roy, S. R. See Singh and Roy (1972)
Hoy, S. R., and Singh, P. N. (1977). A plane symmetric universe filled with disordered radiation,
J. Phys. A10, 49. See § 13.6.
Roy, S. R11 and Tripathi, V. N. (1972). Cylindiically symmetric electromagnetic field of the second class, Indian J. Pure & Appl. Hath. 3, 926. See § 20.4.
Ruban, V. A, (1978). The dynamics of the spatially homogeneous (axisymmetric) cosmological models. II, Preprint not. 412, Leningrad. See § 12.3,, 12.4.
Ruffini, R, See Parker et al. (1973)
Russell-Clarkj R. A. See d’Invemo and RnsselI-CIark (1971), Gibbons and Russcll-Clark (1973)
Hyan, M. P,, and Shepley, L. 0. (1975). Homogeneous Relativistic Cosmologies, Princeton Univ. Press. Set §§ 10.4.) 11.2., 11.3.
Sachs, R. K. (1962). Gravitational waves in general relativity. VIII, Waves in asymptotically flat space-time, Proc. Roy. Soc. A 270, 103. See § 25.1.
Sachs, R. K. See also Goldberg and Sachs (1962), Jordan et al. (1961), Kantowski and Sachs
(1966)
Rackfield. A, (1971). Physical ivlernretatiori ot WT ?»Фч> Proc. Camb. Phil. Soc. 70, 89. Hee S 18.3,
Safko, J. L. (1977). A “superposition” of static, cylindrically symmetric solutions of the Einstein-Maxwell field, Phys. Rev. D 16, 1678. See § 20.2.
Safko, J. L. See also Carlson and Safko (1978)
Sapar, A. (1970). Basic dependences for cosmological models with matter and radiation (in Russian},-Astron. Zh. (USSR) 47, 503. See § 12.2.
Sato, H. See Toraimatsu and Sato (1972, 1973)
Saunders, P. T. (1967). Non-isotropic model universes, Ph. D. Thesis, London. See § 11.3.,
12.4.
Sbytov, Y. G. (1976). Interaction of plane gravitational waves (in Russian), Zh. Eksper. Teor. Fiz. 71, 2001. See § 15.2.
Scanlan, G. See Ludwig and Scanlan (1971)
Schiffer, М. M., Adler, R. J., Mark, J., and Sheffield, C. ?1973). Kerr geometry Os complexified Schwarzschild geometry, J. Math. Phys. 14, 52. See § 30.6.
Schild, A. See Debney et al. (1969), Kerr and Schild (1965, 1967), Plebanski and Schild (1976), Robinson and Schild (1963), Robinson et al. (1969b)
Schimming, R. (1974). Riemannsche Raume mil ebenfronliger und mil ebener Symmetric, Math. Nachr. 59, 129. See § 21.5.
Schmidt, B. G. (1967). Isometry groups with surface-orthogonal trajectories, Z. Naturforsch. 32». 1351. See § 8.6.
Schmidt, B.’ G. (1968). Riemannsche Raume mil mehrfach transitiver Isometriegruppe, Ph. D. Thesis, Hamburg. See §§ 8.6., 9.2., 10.1.
Schmidt, B. G. (1971). Homogeneous Riemannian spaces and Lie algebras of Killing fields, GRG 2, 105. See 8.6.
Schmidt, B. G. See also MacCalIum et al. (1970)
Schmutzer, E. (1968). Relativistische Physik (Klass. Theorie), Teubner, Leipzig. See § 3.6.
Schouten, J. A. (1954). Ricci-Calculus, Springer-Verlag, Berlin, Gottingen, Heidelberg. See §§ 2.8., 3.1.
Sohrank, G. See Thompson and Schrank (1969)
Schiicking, E. See Ozsvith and SchOcking (1962, 1969)
Schwarzschild, K. (1916a). Vber das Gravitationsfeld eines MassenpunkHt uach der Einsteinschen Theorie, Sitz. Preuss. Akad. Wiss., 189. See § 13.4.
.Schwarzschild, K. (1916b). Ober das Gravitationsfeld einer Kugel aus inlompressibler FlHssigbeit nach der Einsteinschen Theorie, Sitz. Preuss. Akad. Wise., 424. See § 14.1.
Sciamtt, D. W. (1961). Recurrent radiation in general relativity, Proc. Camb. Phil. Soc. 57, 430. See § 31.2.
Send, W. (1972). Losungen und a-iymptotischea YtrhaUen einer Klasse von kosmdogischen Modellen, Diplomarbeit, Hamburg. See § 12.4.
Jjengier, J. See Cahen and Sengier (1967)
397
Serdaroglu, M. See Onengut and Serdaroglu (1975)
Sharan, R. See Singh et al. (1965), Singh et al. (1969)
Sharp, D. II. See Misner and Sharp (1964)
Shaw, R. See Collinson and Shaw (1972)
Sheffield, C. See Adler and Sheffield (1973), Schiffer et al. (1973)
Shcpley1 L. C. See Ryan and Shepley (1975)
Shikin, I. S. (1966). Homogeneous anisotropic cosmological mode! with magnetic field (in Russian), Dokl. Akad. Nauk SSSR 171, 73. See § 12.1., 12.3.
Shikin, I. S. (1972). Gravitational fields witk groups of motion on two-dimensional transitivity hypersurfaces in a model with matter and a magnetic field, Commun. Math. Phys. 26, 24. See §11.1.
