Точные решения уравнений Эйнщтейна - Крамер Д.
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Shikin, I. S. (1975). Anisotropic cosmological model of Bianchi type- V in general (axially symmetric) case with moving matter (in Russian), Zh, Eksp. Teor. Fiz. 68, 1583. See §§ 11.4., 12.3.
Siklos, S. Т. C. (1976a). Two completely singularity-free NVT space-times, Phys. LettersA 59, 173. See § 11.3.
Siklos, S. Т. C. (1976b). Singularities, invariants and cosmology, Ph. D. Thesis, Cambridge, See §§ 5.1., 8.2., 9.2., 10.2., 11.2.
Siklos, S: Т. C. (1978). Algebraically special homogeneous space-times, Preprint Univ. of Oxford, See §§ 10.2., 10.5., 11.2., 11.3., 33.2.
Singatullin, R. S. (1973). Exact wave solutions of EinsUin-Maxwell equations defined by Einstein-Boeen solutions (in Russian), Grav. і Teor, Otnbs., Univ. Kazan 9, 67. See § 20.4.
Singh, D. N. See Singh and Singh (1968), Singh et al. (1969)
Singh, K. P., and Abdussattar (1973). Plane-symmetric cosmological model. 11, J. Phys. Л в,
1090. See § 12.4.
Singh, K. P., and Abdussattar (1974). A plant-symmetric universe filled with perfect fluid, Curr. Sci. 48, 372. See § 12.4.
Singh, K. P., and Roy, S. R. (1972). Classification of electromagnetic fields, Indian J. Pure
& Appl. Math. 8, 532. See § 5.2.
Singh, K. P., and Singh, D. N. (1968). A plane symmetric cosmological model, Mon. Not. Roy, Astr. Soc. 140,453. See $ 12.4.
Singh, K. P., Radhakrishna, L., and Sharan, R. (1965). Electromagnetic fields and cylindrical symmetry, Ann. Phys. (USA) 82, 46. See § 20.4.
Singh, K. P., Sharan, R., and Singh, IX N. (1969). Scalar differential invariants in general relativity, Proc. Nat, Inst, Sci. India А Зо, 94. See § 31.4.
Singh, P. N. See Roy and Singh (1977)
Singh, R. A.' See Misra and Singh (196T)
Sistero, R. F. (1972). Belativistic non-zero pressure cosmology, Astrophys. & Space Sci. 17, 150. See § 12.2.
Skripkin, V. A. (1960). Point explosion in an ideal incompressible fluid in the general theory of relativity (in Russian), Dokl. Akad, Nauk SSSR186,1072. See § 14.2.
Sneddon, G. E. (1975). Change of Petrov type Vnder generation of solutions of Einstein's equations, J. Math. Phys. 16, 740. See § 30.5,
Sneddon. G. E. (1976). Hamiltonian cosmology! A further investigation, J. Phys. A 9, 229. See § 11.2.
Som, М. M. See Teixeira et al. (1977 a, b)
Sommers, P. (1973). On Killing tensors and constants of motion, J. Math. Phys. 14, 787. See § 31.3.
flommers, P. (1976). Properties of shear-free congruences of n«8 geodesics, Proc. Roy. Soc. -' bond. A 84», 309. See § 25.6.
Sommers, P, (1977). Type N vacuum space-times as special functions in Ct, GRG 8, 855. See §25.3,
Sommers, P. See also Hughston and Sommers (1973), Hughston et al. (1972)
Sommers, P., and Walker, M. (1976). A note on Hauser's type N gravitational field with twist, J. Phys. A », 357. See $ 25.3.
Spanos, J. T. J. See Israel and Spanos (1973)
Spelkens, J. See Cahen nnd Spelkens (1967)
Srivastava, D. C. See Misra and Srivastavft (1973, 1974)
Stftchel, J. J. (196$), Cylindrical gravitational news, J, Math. Phys. 7, 1321. See § 20.3..
398
Stachel, J. See also PIebanski and Stachcl (1968), Goenner and Stachel (1970)
Stephani, H. (1967 a). Vber Losungen der Einsteinschen Feldgleichungenf die sick in einen funfdimensionalen flachen Raum einbetten Iasseni Commun. Math. Phys. 4, 137. See § 32.4. Stephanit H. (1967 b). Konform flache GravUationsfelder, Commun. Math. Phys. 6,337. See § 32.5. ^tephani, K. (1968). Kinige Losungen der Einsteinschen Feldgleichungen mit idealer FlHssigheitf die sich in einen funfdimensionalen flachen Raum einbetten Iassent Commun. Math. Phys. 9, 53. See § 32.4.
Stephani, H. (1978). A note on Killing tensors, GRG 9, 789. See § 31.3.
Stephani, H. (1979). A method to generate algebraically special pure radiation field solutions from the vacuum, J. Phys. A 12, 1045. See § 26.6.
Stephani, H. See also Kramer et al. (1972)
Sternberg, S. (1964). Lectures on Differential Geometry, Prentice-Hal!, Englewood Cliffs, N.J.
See §§ 2.1., 2.7.
Stewart, J. M. See MaeCallum et al. (1970)
Stewart, J. M., and Ellis, G. F. R. (1968). Solutions of Einstein's equations for a fluid which exhibit local rotational symmetry, J. Math. Phys. 9, 1072. See §§ 9.2., 11.1., 11.2., 11.4., 29.1.,
29.2., 29.3.
Stewart, J. M., and Walker. M. (1973). Black holes: the outside story, Springer Tracts in Modern Physics 69, Springer Verlag, Berlin, Heidelberg, New York. See § 18.5,
Stoker, J. J. (1969). Differential Geometry, Pure and Applied Math. A Series of Texts and Monographs, Wiley, NewYork—London—Sidney — Toronto. See §2.1.
Strauss, H. See Robinson et al. (1969b)
Strunz, H. C. (1974). On the problem of the determination of general relativistic spaces by their scalar differential invariants, Ph. D. Thesis, Univ. of Washington. See §31.4.
Suhonen, E. (1968). General relativistic fluid sphere at mechanical and thermal equilibrium, Kgl. Danske Vidensk. Sels., Mat.-Fys. Medd. Зв, I. See § 14.1.
