Contents

660 ReferencesLi, W.and Ernst, F.J.(1989).A family of electrovac colliding wave solutions ofEinstein’s equations.JMP 30, 678.See §§25.5, 34.1.Li, W., Hauser, I. and Ernst, F.J. (1991a). Colliding gravitational plane waves withnoncollinear polarizations.JMP 32, 723.See §25.4.Li, W., Hauser, I. and Ernst, F.J. (1991b). Colliding gravitational waves withKilling–Cauchy horizons.JMP 32, 1025.See §25.4.Li, W., Hauser, I. and Ernst, F.J. (1991c). Colliding wave solutions of the Einstein–Maxwell field equations.JMP 32, 1030.See §25.5.Li, W., Hauser, I. and Ernst, F.J. (1991d). Nonimpulsive colliding gravitational waveswith noncollinear polarizations.JMP 32, 2478.See §25.4.Li, W.and Hou, Bo-yu (1989).The Riemann–Hilbert transformation for an approachto a representation of the Virasoro group.JMP 30, 1198.See §10.7.Liang, Can-Bin (1995).A family of cylindrically symmetric solutions to Einstein–Maxwell equations.GRG 27, 669.See §22.4.Lichnerowicz, A.(1955).Théories relativistes de la gravitation et de l’électromagnétisme(Masson, Paris).See §§3.8, 18.1.Liddle, A.and Lyth, D.(2000).Cosmological inflation and large-scale structure(Cambridge University Press, Cambridge).See §14.1.Lifshitz, E.M. and Khalatnikov, I.M. (1963). Investigations in relativistic cosmology.Advances Phys. 12, 185.See §13.3.Lind, R.W. (1974). Shear-free, twisting Einstein–Maxwell metrics in the Newman–Penrose formalism.GRG 5, 25.See §§7.1, 27.1, 30.3.Lind, R.W. (1975a). Gravitational and electromagnetic radiation in Kerr–Maxwellspaces.JMP 16, 34.See §§30.4, 30.6.Lind, R.W. (1975b).Stationary Kerr–Maxwell spaces.JMP 16, 39.See §30.4.Lindblom, L.(1980).Some properties of static general relativistic stellar models.JMP21, 1455.See §18.6.Lindblom, L.(1981).Some properties of static general relativistic stellar models.II.JMP 22, 1324.See §18.6.Linet, B.(1987).A charged black hole and a cosmic string in equilibrium. CQG 4, L33.See §18.7.Lor, J.C. and Rozoy, L. (1991). The Ricci curvatures of a Riemannian or pseudo-Riemannian manifold do not always determine its metric.(in French).HelveticaPhys. Acta 64, 104.See §9.2.Lorencz, K.and Sebestyén, A.(1986).On a fourth-order equation of axisymmetricstationary vacuum spacetimes, in Proceedings of the fourth Marcel Grossmannmeeting on general relativity, ed.R.Ruffini, page 997 (North-Holland,Amsterdam, Netherlands).See §19.5.Lorenz, D.(1981).Tilted electromagnetic Bianchi type I and type II cosmologies.Phys.Lett. A 83, 155.See §14.3.Lorenz, D.(1982a).Exact Bianchi type I solutions with a cosmological constant.Phys.Lett. A 92, 118.See §14.4.Lorenz, D.(1982b).On the solution for a vacuum Bianchi type-III model with acosmological constant.J. Phys. A 15, 2997.See §14.3.Lorenz, D.(1983a).Exact Bianchi–Kantowski–Sachs solutions of Einstein’s fieldequations.J. Phys. A 16, 575.See §14.3.Lorenz, D.(1983b).On the general vacuum solution with a cosmological constant forBianchi type-VI 0.Acta Phys. Polon. B 14, 479.See §13.3.Lorenz, D.(1983c).Spatially self-similar cosmological model of Bianchi type- 1I.Astrophys. Space Sci. 93, 419.See §15.7.Lorenz-Petzold, D.(1984).On the general vacuum and stiff matter solutions for‘diagonal’ Bianchi type-VI 0 and type-VII 0 models. Acta Phys. Polon. B 15, 117.See §§13.3, 14.4.