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References 629Cosgrove, C.M. (1982b). Relationship between the inverse scattering techniques ofBelinskii–Zakharov and Hauser–Ernst in general relativity. JMP 23, 615. See§34.7.Covarrubias, G.M. (1984). A class of Szekeres space-times with cosmological constant.Astrophys. Space Sci. 103, 401.See §33.3.Cox, D.and Flaherty, E.J.(1976).A conventional proof of Kerr’s theorem.Commun.Math. Phys. 47, 75.See §32.1.Cox, D.and Kinnersley, W.(1979).Yet another formulation of the Einstein equationsfor stationary axisymmetry.JMP 20, 1225.See §§19.5, 22.3.Crade, R.F. and Hall, G.S. (1982). Second order symmetric tensors and quadraticsurfaces in general relativity.Acta Phys. Polon. B 13, 405.See §5.1.Crampin, M. and Pirani, F.A.E. (1986). Applicable differential geometry.LondonMathematical Society lecture notes, vol.59 (Cambridge University Press,Cambridge).See §2.11.Cruzate, J., Diaz, M., Gleiser, R.J and Pullin, J.A. (1988). Soliton collision incosmologies with matter.CQG 5, 883.See §25.6.Curry, C.and Lake, K.(1991).Vacuum solutions of Einstein’s equations in double-nullcoordinates.CQG 8, 237.See §15.4.Curzon, H.E.J. (1924). Cylindrical solutions of Einstein’s gravitational equations. Proc.London Math. Soc. 23, 477.See §20.2.Czapor, S.R. and Coley, A.A. (1995). Diagonal G 2 spacetimes admitting inheritingconformal Killing vector fields.CQG 12, 1995.See §§14.4, 23.3, 35.4.Czapor, S.R. and McLenaghan, R.G. (1982). Orthogonal transitivity, invertibility andnull geodesic separability in type D vacuum solutions of Einstein’s field equationswith cosmological constant.JMP 23, 2159.See §26.2.da Costa, J. and Vaz, E.G.L.R. (1992). Vacuum type N space-times admittinghomothetic vector fields with isolated fixed points.GRG 24, 745.See §8.7.D¸abrowski, M.and Stelmach, J.(1986).Analytic solutions of Friedman equation forspatially opened universes with cosmological constant and radiation pressure.Ann. Phys. (USA) 166, 422.See §14.2.Daftardar-Gejji, V.(1998).A generalization of Brinkmann’s theorem.GRG 30, 695.See §3.7.Dagotto, A.D., Gleiser, R.J. and Nicasio, C.O. (1991). On the Khan–Penroseconstruction for colliding electro-vacuum plane waves.CQG 8, 2085.See §25.5.Dagotto, A.D., Gleiser, R.J. and Nicasio, C.O. (1993). Two-soliton solutions of theEinstein–Maxwell equations.CQG 10, 961.See §34.5.Daishev, R.A. (1984). Homogeneous solutions of Einstein’s equations for perfect liquid.Ukrayins’kyi Fiz. Zh. 29, 1163.See §13.4.Dale, P.(1978).Axisymmetric gravitational fields: a nonlinear differential equationthat admits a series of exact eigenfunction solutions. Proc. Roy. Soc. Lond. A362, 463.See §20.6.Darmois, G.(1927).Les équations de la gravitation einsteinienne.Mémorial dessciences mathématique, part XXV (Gauthier-Villars, Paris).See §§3.8, 20.2.Das, A.(1979).On the static Einstein–Maxwell field equations.JMP 20, 740. See §18.6.Das, K.C. (1980a). Axially symmetric solutions in general relativity. J. Phys. A 13,2985.See §21.1.Das, K.C. (1980b).Electrovac solution.J. Phys. A 13, 223.See §21.1.Das, K.C. (1983). New sets of asymptotically flat static and stationary solutions. PRD27, 322.See §20.6.Das, K.C. (1985). Odd-soliton solutions of the Einstein equations in a vacuum. PRD31, 927.See §34.5.Das, K.C. and Chaudhuri, S. (1991). Soliton solution of Einstein field equations fromnondiagonal seed.Indian J. Pure Appl. Math. 22, 963.See §34.5.

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