Точные решения уравнений Эйнщтейна - Крамер Д.
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Osinovsky, М. E. See Klekowska and Osinovsky (1973)
Ozsvath, I. (1965a). All homogeneous solutions of Einstein's field eqvations teith incoherent matter and electromagnetic radiation, 3. Math. Phys. 6, 1265. Set § 10.5.
Ozsvath, I. (1965b). New homogeneous solutions of Einstein’s field equations with incoherent mutter, Akad. Wise. Lit. Mainz, Mnth.-Nat. Kl, 1965 no. I. See §§ 10.4., 10.5.
OzsvAth, I. (1965c). Womogeneous solutions of the Einstein-MaxuieU equations, 3. Math. Phys, 6, 1255. See § 10.3.
Ozsvith, I. (1965d). New homogeneous solutions of Einstein’s field equations with incoherent matter obtaintd by a spinor technique. 3. Math. Phys. 6, 590. See $ 10.4.
Ozsvath, I. (1966). TwO rotating universes with dust and electromagnetic field, in: Hoffmann, B. (Ed.), Perspectives in Geometry and Relativity, Indiana XTniversity Press p. 245. See §§ 10.5., 11.1.
Ozsv&th, I. (1970). Dust-filled universes of class H and class III, 3. Math. Phys. 11, 2871. See § 10.4.
Ozsvath. I. (1977). Spatially homogeneous Lichnerowicz universes, GR6 8, 737. See $ 12.1.
Ozsvath. I. See also Hiromoto and Ozsvith (1978)
Ozsvath, I., and SchQcking, E. (1962), An anti-Mach metric, in : Recent Developments in ¦ General Relativity, Pergamon Press — PWN, p. 339. See § 10.2.
Ozsvath, I., and Schucking, E. (1969), The finite rotating universe, Ann. Phys. (USA) 65, 166. See § 10.4.
Pandey, D. B. See Misra and Pandey (1973)
Pandya, I. M., and Vaidya, P. C. (1961), Wave solutions in general relativity. I, Proc. Nat.
” Inst. Sci. India A 27, 620. See § 27.5.
Papapctrou, A. (1947). A static solution of the equations of the gravitational field for an arbitrary charge distribution, Proc. Roy. Irish Acad. A 51, 191. See §§ 16.7., 19.1.
Papapetrou, A. (1953). Eine rotationssymmetrische Losung in der AUgemeinen Relativitatstheorie, Annalen Physik 13. 309. See § 18.3.
Papapetrou, A. (1963). Quelques remarques sur Ies champs gravitationneU stationnaires, C.R. Acad. Soi. (Paris) 257, 2797. See § 16.4.
Papapetrou, A. (1966). Champs gravitationnels stationnaires a symitrie axiale. Ann. Inst. H. Poincaгё A 4, 83. Set §§ 17.2., 17.3., 20.3.
Papapetrou, A. (1971a). Queiques remarques sur Ie formalisme de Newman-Penrose, C.R. Acad. Sci. (Paris) A 272, 1537. See § 7.2.
Papapetrou, A. (1971b). Les relations identiques entre Ies Equations du formalisme de Newman-Penrose, C.R. Acad. Sci. (Paris) A 272, 1613. See § 7.2.
Parker, L. See Kobiske and Parker (1974)
Parker, L., Ruffini, R,, and Wilkins, D. (1973), Metric of two spinning charged sources Ili equilibrium, Phys. ReT. B 7, 2874, See f 19.1.'
Patel, L. K. See Yaidya and Patel (1973)
Patel, L. K., and Yaidyaj P. C. (1999). Qa plane-symmeirk cosmological models. Progress of Math. 3, 158, Sei § 12.4.
394
Patera, J., and Winternitz, P. (1977). Subalgebras of real three and four-dimensional Lie aigebras, J. Math. Phys. 18, 1449. -See § 8.2.
Patnaik, S. (1970). Einstein-Maxweil fields with plane symmetry, Proc. Camb. Phil. Soc. 67| 127. See § 13.4.
Peebles, P. J. (1971). Physical Cosmology, Princeton Univ. Press. See § 12.1.
Penrose, R. (1960). A spinor approach to general relativity, Ann. Phys. (USA) 10, 171. «See §§ 3.6., 4.3.
Penrose, R. (1965). A remarkable property of plane waves in general relativity, Rev". Mod. Phys.
37, 215. See § 32.7.
Penrose, R. (1968). Structure of space-time, in: DeWitt, C. SI., and Wheeler, J. A. (Eds.) Battelie Rencontre, 1967 Lectures in Math, and Phys., Chapter VII, Benjamin, New York, Amsterdam. See §§ 3.6., 4.3.
Penrose, R. (1972). Spinor classification of energy tensors, Gravitataiya, Nauk dumka, Kiev, p. 203. See § 6.1.
Penrose, R. See also Geroch et al. (1973), Hughston et al. (1972), Khan and Penrose (1971), Newman and Penrose (1962), Walker and Penrose (1970)
Peres, A. (1960a). Invariants of general relativity. II. Classification of spaces, N. Cim. 18, 36. See §5.1.
Peres, A. (1960b), Null electromagnetic fields in general relativity theory, Phys. Rev. 118, 1105. See § 21.5.
Perjes, Z. (1968). A method for constructing certain axially-symmetric Einstein-Maxwell fields, N. Cim. B 56,600. See § 19.1.
Perjes, Z. (1970), Spinor treatment of stationary space-times, J. Hath. Phye. 11, 3383. See § 16.5.
Perjes, Z. (1971). Solutions of the coupled Einstein-Maxwell equations representing the fields of spinning sources, Phys. Rev. Lett. 27, 1668. See § 16.7.
Perj6s, Z. (1976). Introduction to spinors and Petrov types in general relativity, Acta Phys. Acad.
Sci. Hung. 41, 173. See § 4.3.
Perjes, Z. See also Kota and Perjes (1972), Lukacs and Perjes (1973)
Petrov, A. Z. (1962). Gravitational field geometry as the geometry of automorphisms, in: Recenb Developments in General Relativity, Pergamon Press — PWN, p. 379. See §§ 10.2., 27.5. Petrov, A. Z. (1963a). Types of field and energy-momentum tensor (in Russian), TJchonie Zapiski K a tan. Gos. Univ. 123, 3. See § 5.1.
