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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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Petrov, A. Z. (19631)). On Birkhaf/’s Theorem (in Russian), Uchonie Zapiski Kazan. Gos. Univ. 128, 61. See § 13.4.

Petrov, A. Z. (1963c). Central-symmetric gravitational fields (in Russian), Zh1 Eksper. Teor. Fiz. 44, 1525. See § 13.4.

Petrov, A. Z. (1966). New methods in General Relativity (in Russian), Naukaf Moscow. [English edition of Petrov’s book: Einstein spaces, Pergamon Press (1969)]. Set §§4.2., 8.1., 8.2.,

8.4., 8.5.,9.1., 10.5., 11.1., 15.1., 20.3., 21.1., 31.1., 31.3., 31.4.

Pirani, F. A. E. (1957). Invariant formulation of gravitational radiation theory, Phys. Rev. 105,

1089. See § 4.3.

Pirani, P. A. E. (1965). Introduction to gravitational radiation theory, in: Brandeis (1964) Lectures on General Relativity, vol. I, Prentice-Hall, Englewood Cliffs., New Jersey, p. 249. See §§ 3.6., 7.2.

Pirani, F. A. E. See also Bondi et al. (1959)

Plebanski, J. (1964). The algebraic structure of the tensor of matter, Acta Phys. Polon. 26, 963. See § 5.1.

Plebanski, J. (1967). On conformally equivalent Riemannian spaces, Centro de investigation у de estudios, Mexico. See § 8.5.

Plebaiiski, J. (1975). A class of solutions of Einstein-Maxwell equations, Ann. Phys. (USA) 90, 196. See § 19.1.

Plebanski, J. (private communication). Solutions of Einstein equations Gfl, = -QKjlK, determined by the condition that Kfl is the quadruple Debever-Penrose vector. See § 22.1.

Plebanski, J. See also Hacyan and Plebanski (1975), Kowalczynski and Plebanski (1977) Plebanski, J., and Demianski, M. (1976). Rotating, charged and uniformly accelerating mass in general relativity, Ann. Phys. (USA) 98, 98. See §§ 19.1., 25.5.

Plebanski, J., and Hacyan, S. (1979). Some exceptional electro-vac type D metrics with COtmo-togical constant, J. Math. Phye. 20,1004. See § 22,1.

395
Plebanski, .1., and Starhel, J. (1968). Einstein tensor and spherical symmetry, Jr.-Math. Phys. 9, 269. See §§ 5.1.. 13.4.

Plebanski, J., and Schild, A. (1976). Complex relativity and double KSmetrics, N. Cim. B 35,35. See § 28.5.

Polishchuk, R. K. (1970). Pelrov classification of gravitational fields and ehronometrical Mt. variants (in Russian), Vestn. Moak. Univ. Fiz. Astr. ft, 860. See §4.2.

Prakash. A. See Newman et al. (1965)

Prasad, H. See Lai and Prasad (1969)

lQvist, B. See Kustaanheimo and Qvist (1948)

Kadhakrishna, L. (1963). Some exact non-static cyliniricaUy symmetric electrovac universes, PtOtt Nat. Inst. Sci. India A 29, 588. See § 20.4.

Radhakrishna1 L. See also Misra and Radhakrishna (1962), Singh et al. (1965)

Rainich, G. Y. (1925). Electrodynamics in general relativity. Trans. Amer. Math. Boo. 87» 100» See § 5.4.

Rastall1 P. (1960). A solution of the Einsteinfield equations, Oftn&d. J. Phys. 88,1661, See S 16.4. Ray, J. R. See Lauten III and Ray (1975, 1977)

Ray, J. R., and Thompson, E. L. (1975). Space-time symmetries and the complexion of the electromagnetic field, J. Math. Phys. 16, 345. See § 9.1.

Ray, J. R., and Wei, M. S. (1977). A solution-generating theorem with applications in general relativity, N. Cim. B 48, 151. See § 30.5.

Raychaudhuri1 A. (1955). Belativistic cosmology, I., Phys. Rev, 98, 1123. See § 6.2. Raychaudhuri, A. (1958). An anisotropic cosmological solution in general relativity, Proo. Phjl.

Soc. Lond. 72, 263. See § 12.4.

Raychaudhuri, A. (1975). Spherically symmetric charged dust distributions in general relativity, Ann. Inst. H. Poincare 32, 229. See § 13.5.

Reina, C., and Treves, A. (1975). Gyromagnetic ratio of EinAein-Ztaxwell fields, Phys. Rev. D 11, 3031. See S 30.5.

Rcissner1 H. (1916). Vber die Eigengravitalion des elektrischen Feldes naeh der Einsteinschen Theoriey Annalen Physik 50, 106. See §§ 13.4., 19.1.

Reuse, J.-D. (1968). Un champ gravitationnel cylinirique et non stationnafre, C.R. Acad. Soi» (Paris) A 266, 794. See § 20.3.

. Robertson, H. P. (1935). Kinematics and world-structure, Astrophys. J. 88, 284. See J 10.1. Robertson, H. P. (1936). Kinematics and world-structure, Astrophys. J. 83,137» See § 10.1. Robinson, В. B. (1961). Rdalivistic universes with shear, Proo. KatT. Aoad. Sci. U.S. 47, 1862. See § 12.4.

Robinson, I (1959). A solution of the Einstein-Maxwell equations, Bull. Aead. Polon. Sei., Ser, Math. Astr. Phys. 7, 351. See §§ 10.3., 19.1.

Robinson, I. (1961). Null electromagnetic fields, J. Math. Phys. 2, 290. See § 7.6.

Robinson, I. (1975). On vacuum, metrics of type (3,1), GRG 6, 423. See §§ 24.1., 25.2., 26.4. Robinson, I. See also Bondi et al. (1959)

Robinson, I., and Robinson, J. R. (1969). Vacuum metrics without symmetry, Int. J. Theor.

Phys. 2, 231. See §§ 26.1., 26.2., 26.4.

Robinson, I., and Schild, A. (1963). Oeneralization of a theorem by Ooldberg and Sachs, J. Math. Phys. 4, 484. See § 7.5.

Robinson, I., and Trautman, A. (1962). Some spherical gravitational wave» in general relativity, Proc. Roy. Soc. Lond. A 266, 463. See §§ 23.1., 23.2., 24.1., 24.2.

Robinson, I., Robinson, J. R., and Zund, 'J. D. (1969a). Degeneraie gravitational fields with twisting rays, J. Math. Mech. 18, 881. See §§ 23.1., 25.1.
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