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Точные решения уравнений Эйнщтейна - Крамер Д.

Крамер Д., Штефани Э., Херльт М., Мак-Каллум М. Точные решения уравнений Эйнщтейна — М.: Энергоиздат, 1982. — 416 c.
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Sulaiinan. A. H. See Bonnor et al (19/7)

Sust, M. See Neugebauer and Sust (1975)

Swaminaraynn, N. S. See Bonnor and Swaminarayan (1964, 1965)

Synge, J. L. (1960), Relativity: The General Theory, North-HolIand, Amsterdam. See § 16.5.

Synge, J. L. (1964). The Petrov classification of gravitational fields, Commun. Dublin Inst.

Adv. Stud. A, no. 15. See §§4.1., 4.2.

Szafron, D. A. (1977). Inhamogeneous cosmologies: New exact solutions and their evolution, J.

Math. Phys. 18, 1673. See § 29.3.

Szafron, D. A., and Wainwright, J. (1977). A class of inhomogeneous perfect fluid cosmologies, J. Math. Phys. 18, 1668. See §29.3.

Szekeres, G. (1960). On the singularities of a Riemannian manifold. Publ. Mat. Debrecen 7, 285. See § 13.4.

Szekeres, P. (1963). Spaces conformal to a class of spaces in general relativity, Proc. Roy. Soc.

Lond. A 274, 206. See § 3.7.

Szekeres, P. (1966a). Embedding properties of general relativistic manifolds, N. Cim. 48, 1062.

See § 32.3.. 32.6.

Szekeres, P. (1966b). On the propagation of gravitational fields in matter, J. Math. Phys. 7, 751. See §§3.5., 7.5., 22.1., 27.7., 29.4.

Szekeres, P. (1968). Multipole particles in equilibrium in general Telativityi Phys. Rev. 176, 1446. See § 18.1.

Szekeres, P. (1970). Colliding gravitational waves, Nature 228, 1183, See § 15.2-Szekeres, P. (1972). Colliding plane gravitational waves, J. Math. Phys. 13, 286. See § 15.2. Szekeres, P. (1975). A class of inhomogeneous cosmological models, Commun* Math. Phys, 41, 55. See § 29.3.

Szekeres, P. See also Be'J nnd Szekeres (1972, 1974)

Tabensky, R. R. See Letelier and Tabensky (1974* 1975a, b), Melnick and Tabensky (1975) Tabcnsky, R. R., and Taub, A. H. (1973). Plane symmetric self-gravitating fluids with pressure equal to energy density, Conwn. Math. Phys. 29, 61, See § 13.6., 15.1*

Takeno, H. (1961). The mathematical theory of plane gravitational waves in general relativity, Sci. Rep. Res. Inst. Theor. Phys. Hiroshima Univ. no. I. See § 21.5.

Tfckeno, H. (1966). The theory of spherically symmetric space-timesr Sci. Rep, Res. Inst, Theor. Phys. Hiroshima Univ. no. 5. See § 13.1,

399
Takeno, H., and Kitemura, S. (1968). On the space-time admitting a parallel null vector IieUlt Tensor 19, 207. See § 6.2.

Takeno, H., and Kitemura, S. (1969). On the Binetein tensors of spherically symmetric space-times. Progress of Math. 8, 7. See § 13.1.

Talbot, C. J. (1969). Neuman-Pemrose approach to twisting degenerate metrics, Commun. Math.

Phys. 13, 45. See §§ 7.1., 23.1,, 30.6.

Tamburino, L. See Newman and Tamburino (1962), Newman et al. (1963)

Tanabe, Y. (1974). A comment on physical interpretation of the Tomimatsu-Sato metrics, Prog.

Theor. Phys., 62, 727. Set $ 18.5.

Tanabe, Y. (1977). SU(2,1) symmetry of the Einstein-Maxwell fields, Prog. Theor. Phys. 57, 840. See § 30.3.

Tanabe, Y. (1978). Exact solutions of the stationary axisymmetric Emstein-Maxwell equations, Prog. Theor. Phys. «0,142. See § 30.3.

Tariq, N. See McLenaghan and Tariq (1975), McLenaghan et al. (1975)

Tariq, N., and Tapper, B. 0. J. (1975). A class of algebraically general solutions of the Einstein-Maxwell equations for non-null electromagnetic fields, GBG в, 345. See § 11.2.,.11.3.

Taub, A. H. (1951). Empty space-times admitting a three parameter group of motions, Ann.

Math. 68, 472. See §§ 11.2., 11.3., 13.4.

Taub, A. H. (1956). Isentropic hydrodynamics in фіапе symmetric space-times, Phye. Rev. 103, 454. See § 13.6.

Taub, A. H. (1968). Restricted motions of gravitating spheres. Ann. Inst. H. Poincart A 9, 153. See § 14.2.

Taub, A. H. (1972). Plane-symmetric similarity solutions for self -gravitating fluids, in: O’Rai-feartaigh, L. (Ed.), General Relativity (Papers in Honour of J. L. Synge), Clarendon Press, Oxford, p. 133. See § 13.6.

Taub, A. H, (1976). High frejuency gravitational radiation in Kerr-Schild space-times, Commun.

Math. Phys. 47, 185. See § 24.3.

Taub, A. H. See also MacCaIIum and Taub (1972), Misner and Tuub (1968), Tabensky and Taub (1973)

Tauber, G. E. (1957). The gravitational fields of electric and magnetic dipoles, Canad. J. Phys, 36, 477. See § 19.1.

Tauber. G. E. (1967). Expanding universe in conformally flat coordinates, 3. Math. Phys. 8, 118. ,SVe § 12.2.

Teixeira, A. F. da P., Wolk, I., and Som, М. M. (1977a). Exact relativistic cylindrical solution of disordered radiation, N. Cim. B 41, 387. See § 20.2.

Teixeirn, A. F. da P., Wolk, I., Som, М. M. (1977b). Exact relativistic solution of disordered radiation with planar symmetry, J. Phys. A10, 1679. See § 13.6.

Thompson, A. (1966). A class of related space-times, Tensor 17) 92. See § 28.5.

Thompson, A. See also Kundt and Thompson (1962)

Thompson, E. L. See Ray and Thompson (1975)

Thompson, I. H., and Whitrow, G. J. (1967). Time-dependent internal solutions for spherically symmetrical bodies in general relativity, Mon. Not, Roy. Astr. Soc. 136, 207. See § 14.2. Thompson, J., and Schrank, G. (1969). Algebraic classification of four-dimensional Riemann spaces, J. Math. Phys. 10, 766. See § 5.1.
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