Contents

650 ReferencesIvanov, B.Y. (1999). Expanding, axisymmetric, pure-radiation gravitational fields witha simple twist.PRD 60, 104005.See §30.7.Ivanov, G.G. (1977). An exact solution of Einstein’s equation that describes sphericalgravitational and electromagnetic waves (in Russian).Grav. Teor. Otnos. 12, 69.See §28.2.Iyer, B.R. and Vishveshwara, C.V. (1983). Magnetization of all stationary cylindricallysymmetric vacuum metrics.JMP 24, 1568.See §34.1.Jackson, J.C. (1970).Infilling for NUT space.JMP 11, 924.See §21.2.Jacobs, K.C. (1968). Spatially homogeneous and Euclidean cosmological models withshear.Astrophys. J. 153, 661.See §§14.3, 14.4.Jacobs, K.C. (1969). Cosmologies of Bianchi type I with a uniform magnetic field.Astrophys. J. 155, 379.See §§13.3, 14.1, 14.4.Jantzen, R.T. (1980a). Soliton solutions of the Einstein equations generated fromcosmological solutions with additional symmetry. Nuovo Cim. B 59, 287. See§§10.11, 22.3.Jantzen, R.T. (1980b). Variation of parameters in cosmology. Ann. Phys. (USA) 127,302.See §14.1.Jantzen, R.T. (1983). Uniformly accelerated particle metrics obtained by solitontechniques.GRG 15, 115.See §34.5.Jantzen, R.T. (1984). Spatially homogeneous dynamics: A unified picture, in Cosmologyof the early universe, eds.R.Ruffini and L.-Z.Fang, page 233 (WorldScientific, Singapore).See §13.2.Jantzen, R.T. (1986). Rotation in cosmology: Comments on ‘Imparting rotation toa Bianchi type II space-time,’ by M.J. Reboucas and J.B.S. d’Olival (J.Math.Phys.27, 417 (1986)) and similar papers.JMP 27, 2748.See §13.2.Jantzen, R.T. (1988).Power law time lapse gauges.PRD 37, 3472.See §13.2.Jantzen, R.T.and Rosquist, K.(1986).Adapted slicings of space-times possessingsimply transitive similarity groups.JMP 27, 1191.See §13.2.Jantzen, R.T. and Uggla, C. (1998). The kinematical role of automorphisms in theorthonormal frame approach to Bianchi cosmology.JMP 40, 353.See §13.2.Joly, G.C. and MacCallum, M.A.H. (1990). Computer-aided classification of the Riccitensor in general relativity.CQG 7, 541.See §9.3.Joly, G.C., MacCallum, M.A.H. and Siklos, S.T.C. (1992). Comment on the ‘generalizedaxisymmetric spacetimes’ of Bampi and Cianci. CQG 9, 795. See §§24.3,31.5.Jordan, P., Ehlers, J. and Kundt, W. (1960). Strenge Lösungen der Feldgleichungen derAllgemeinen Relativitätstheorie. Akad. Wiss. Lit. Mainz, Abhandl. Math.-Nat.Kl. 2.See §§9.1, 18.1, 22.1, 24.5.Jordan, P., Ehlers, J. and Sachs, R.K. (1961). Beiträge zur Theorie der reinen Gravitationsstrahlung.Akad. Wiss. Lit. Mainz, Abhandl. Math.-Nat. Kl. 1. See §§4.3,6.1.Jordan, P.and Kundt, W.(1961).Geometrodynamik im Nullfall.Akad. Wiss. Lit.Mainz, Abhandl. Math.-Nat. Kl. 3.See §5.4.Joseph, V.(1966).A spatially homogeneous gravitational field.Proc. Camb. Phil. Soc.62, 87.See §13.3.Julia, B.and Nicolai, H.(1995).Null Killing vector dimensional reduction and galileangeometrodynamics.Nucl. Phys. B 439, 291.See §34.1.Kac, V.G. (1990). Infinite dimensional Lie algebras (Cambridge University Press,Cambridge).See §10.4.Kaigorodov, V.R. (1962). Einstein spaces of maximum mobility (in Russian). Dokl.Akad. Nauk SSSR 7, 893.See §§12.5, 38.2.Kaigorodov, V.R. (1967). Exact type III solutions of the field equations R ij = 0 (inRussian).Grav. Teor. Otnos., Univ. Kazan 3, 155.See §31.5.