Точные решения уравнений Эйнщтейна - Крамер Д.
Скачать (прямая ссылка):
Thorne, K. S. (1967). Primordial element formation, primordial magnetic fields and the isotropy of the universe, Astrophys. 3.148, 51. See §§ 12.1,) 12.3.
Thorne, K. S. See also Misner et al. (1973)
Thorpe, J. A. (1969). Curvature and the Petrov canonical forms, J. Math. Phys. 10, I. See
S 4-2.
Tolman. R. C. (1934a). Effect of inhomogeneity in cosmological models, Proc. Nat. Acad. Sci. U.S. 2«. 69. See 5 13.5.
Tolman. R. C. (1934 b). Relativity, Thermodynamics, and Cosmology, Oxford Univ. Press. See § 12.2.
Tolman, R. C. (1939). Static solutions of Einstein’s field equations for spheres of fluid, Phys.
Rev. 56, 364. See § 14.1.
Tomimatsu, A., and Sato, H. (1972). New exact solution for the gravitational field of a spinning mass, Phys. Rev. Lett. 29, 1344. See § 18.5.
Tomimatsu, A., and Sato, H. (1973). New serim of exact solutions for gravitational fields of spinning masses, Prog. Theor. Phys. 60, 95. See § 18.5,
400
Tomimura, N. (1977). Particular exact inhomogeneous solution with matter and pressure, XT».
Cim. B 42, I. See § 29.3.
Tomimura, N. See also Bonnor and Tomimura (1976), Bonnor et al, (1977)
Tooper, R. F. (1964). General relativistic polytropic fluid spheres, Astrophys. J. 140, 434. See § 14.1.
Torrence, R. See Xewman et al. (1965), Unti and Torrence (1966)
Trautman, A. (1962). On the propagation of information by waves, in: Recent Developments i;> General Relativity, Pergamon Press — PWN, p. 459. See §§ 28.1., 28.2.
Trautman, A. See also Robinson and Trautman (1962)
Treves, A. See Reina and Treves (1975)
Trim, D. W., and Wainwright, D. J. (1974). Nonradiative algebraically special space-times, J. Math. Phys. 15, 535. See §§ 25,1,, 25.2., 26.2., 26.3., 26.4.
Tripathi, V, N. See Roy and Tripathi (1972)
Trollope, R, See Wyman and Trollope (1965)
Triimper, M. (1962). Zur Bemgung von ProbekBrperu in Einsltinschm Gravilalions-Vakuurn--feldem, Z. Phys. 168, 55. See § 16.6.
Triimper, M. (1965). On a special class of type-I gravitational fields, J. Math. Phvs. в, 584. See § 6.2.
Triimper, M. (1967), Einsteinsche Feldgleichungen fiir das axialsymmetrische, stationdre Gravi-tationsfeld im Innern einer »tan rotierenden idealen Flussigkeit, Z. Naturforsch. 22b, 1347. See § 19.2.
Triimper, M. See also Kundt and Triimper (1962, 1966)
Tsoubelis, D. See Harvey and Tsoubelis (1977)
Tupper, B. Ol J. (1976). A class of algebraically general solutions of the Finslein-MaxweU equations for non-null electromagnetic IiMs. II. GRG 7, 479. See § 10.3.
Tupper, B. O. J. See also Dunn and Tupper (1976), McLenaghan et ftl. (1975), Tariq and Tupper (1975)
Unti, T. See Newman and Untj (1963), Newman et al, (1963)
Vnti, T. W. J., and Torrence, R, J, (1966). Theorem on gravitational fields with geodesic rays,.
J. Math. Phys. 7, 535. See § 22.3,
Urbantke, H. (1972). Note on Kerr-Schild Iype vacuum gravitational fields, Acta Phys. Austr..
85, 396. See § 28.2.
Urbantke, H. (1975). Der metrische Ansatz von Trautman, Kerr und Schild rIind einige seiner Anwendungen, Acta Phys. Austr. 41, I. See §§ 22,1., 28.4.
Vaidya, P. C. (1951). The gravitational field of a radiating star, Proc. Indian Acad. Sci. A 33, 264. See § 13.4.
Vaidya, P. C. (1968). Nonstatic analogues of Schwarzschild'з interior solution in general relativity, Phys. Rev. (2) 174, 1615, See § 14.2.
Vaidya, P. C. (1973). Some algebraically special solutions of Einstein’s equations, II., Tensor 27, 276. See § 28.4,
Vaidya, P. C. (1974). A generalized Kerr-Schild solution of Einstein's equations, Proc. Camb.
Phi!, goc. 75, 383. See § 28.4.
Vaidya* P. C. (1977). The Kerr metric in cosmological background, Pramana 8, 512. See § 19.2. Vaidya, P. C. See also Bonnor nnd Vaidya- (1972), Pandya and Vaidya (1961), Patel and Vaidya (1969)
Viiidya1P. C., and Pa tel,),. K. (1973). RndintiviJ Kcrr metric, Phys. Rev. D 7.3590. Sre § 2S.4. Vajk, J. P. (1969). Exnet Hobertnon-Walker cnsMologicnl лоШіоп* containing rclutiristic fluids, J. Math, Phys. 10, 114Г). See 5 12.2.
Vajk, J, P , nnd Eltgroth, P. 0. (1970). Spnlinllj/ homogeneous anisotropic, cosmologknl modeU
containing relativistic fluid nnd magnetic field, J. Math. Phys. 11, 2212. Sec § J2.:5. van iStockum, W. J. (1937). The. gravitational field of a distribution of particles rotating nhunt an axis of symmetry, Proc. Roy. Soc. KcHnhurgh A 57. 135. See §§ 18.4,, 19.2.
Vjokcrs, P. A. (1973). Charged dust spheres in general relativity, Ann. Inst. H. Гоішагс A IS. 137. See § 13.5.
Vishvcshwara, С. V’. See HoenseUtcrs and Visliveshwaia (1978)
Vifhvcshwara, С. V., -and Winirourt J. (1977). Uebilivislically rotating <lusl cylinders, J. Math..
Phys. 18, 1280. See. 19.2., 20.2.
Volkoff, G. M. (1939). On the equilibrium of viassive spheres, Phy Rev. 55, 413.'Set § 14.1.
26—99
401
"Voorhees, В. H. (1970). Static axially symmetric gravitational field*, Pbys. Rev. D 2, 2)19. See § 18.1.
"Voorhoes, B. H. (1972). Electric Weyl spacetimes and the stationary problem, Pbys. Lettem A 8», 114. See §30.5.
