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References 673Quevedo, H.and Mashhoon, B.(1990).Exterior gravitational field of a chargedrotating mass with arbitrary quadrupole moment. Phys. Lett. A 148, 149. See§34.1.Quevedo, H.and Mashhoon, B.(1991).Generalization of Kerr spacetime.PRD 43,3902.See §34.3.Quevedo, H.and Sussman, R.A.(1995).On the thermodynamics of simple nonisentropicperfect fluids in general relativity.CQG 12, 859.See §5.4.Rácz, I.(1997).On Einstein’s equations for space-times admitting a non-null Killingvector.JMP 38, 4202.See §18.3.Rácz, I.and Zsigrai, J.(1996).Generating new perfect-fluid solutions from knownones.CQG 13, 2783.See §§10.11, 21.2.Radhakrishna, L.(1963).Some exact non-static cylindrically symmetric electrovacuniverses.Proc. Nat. Inst. Sci. India A 29, 588.See §22.4.Rainer, A.and Stephani, H.(1999).Similarity reduction of a class of algebraicallyspecial perfect fluids.J. Math. Phys 40, 897.See §33.1.Rainich, G.Y. (1925). Electrodynamics in general relativity. Trans. Amer. Math. Soc.27, 106.See §5.4.Ram, S.(1988).Bianchi type VI 0 space-times with perfect fluid source. JMP 29, 449.See §14.4.Ram, S.(1989a).Generation of LRS Bianchi type I universes filled with perfect fluids.GRG 21, 697.See §14.3.Ram, S.(1989b).Homogeneous Bianchi type VI 0 perfect fluid space-times. Int. J.Theor. Phys. 28, 97.See §14.4.Ram, S.(1989c).LRS Bianchi type I perfect fluid solutions generated from knownsolutions.Int. J. Theor. Phys. 28, 917.See §14.3.Ram, S.(1989d).Spatially homogeneous cosmological models of Bianchi type III.JMP30, 757.See §14.3.Ram, S.(1990).Bianchi type V perfect-fluid space-times.Int. J. Theor. Phys. 29, 901.See §14.4.Ramos, M.P.M. (1998). Invariant differential operators and the Karlhede classificationof type N non-vacuum solutions.CQG 15, 435.See §9.2.Ramos, M.P.M. and Vickers, J.A.G. (1996a). Invariant differential operators and theKarlhede classification of type N vacuum solutions.CQG 13, 1589.See §9.2.Ramos, M.P.M. and Vickers, J.A.G. (1996b). A spacetime calculus based on a singlenull direction.CQG 13, 1579.See §§7.2, 9.2.Ray, D.(1976).Self-gravitating fluids with cylindrical symmetry.JMP 17, 1171. See§10.11.Ray, J.R. and Thompson, E.L. (1975). Space-time symmetries and the complexion ofthe electromagnetic field.JMP 16, 345.See §11.1.Raychaudhuri, A.K. (1955).Relativistic cosmology, I.Phys. Rev. 98, 1123.See §6.2.Raychaudhuri, A.K. (1958). An anisotropic cosmological solution in general relativity.Proc. Phys. Soc. Lond. 72, 263.See §14.4.Raychaudhuri, A.K. (1960). Static electromagnetic fields in general relativity. Ann.Phys. (USA) 11, 501.See §22.2.Raychaudhuri, A.K. and Saha, S.K. (1981).Viscous fluid interpretation of electromagneticfield, I.JMP 23, 2554.See §5.2.Reina, C.and Treves, A.(1975).Gyromagnetic ratio of Einstein–Maxwell fields.PRD11, 3031.See §34.1.Reissner, H.(1916).Über die Eigengravitation des elektrischen Feldes nach derEinsteinschen Theorie.Ann. Phys. (Germany) 50, 106.See §§15.4, 21.1.Reula, O.(1989).On existence and behaviour of asymptotically flat solutions to thestationary Einstein equations.Commun. Math. Phys. 122, 615.See §18.4.Reuss, J.-D. (1968). Un champ gravitationnel cylindrique et non stationnaire. C. R.Acad. Sci. (Paris) A 266, 794.See §22.3.

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