Contents

References 635Ernst, F.J. (1977). A new family of solutions of the Einstein field equations. JMP 18,233.See §20.6.Ernst, F.J. (1978a). Coping with different languages in the null tetrad formulation ofgeneral relativity.JMP 19, 489.See §7.2.Ernst, F.J. (1978b).Generalized C-metric.JMP 19, 1986.See §§17.2, 20.2.Ernst, F.J. (1984). The homogeneous Hilbert problem. Practical application, inSolutions of Einstein’s equations: Techniques and results.Lecture notes in physics,vol.205, eds.C.Hoenselaers and W.Dietz, page 176 (Springer, Berlin).See§34.6.Ernst, F.J. (1994).Fully electrified Neugebauer spacetimes.PRD 50, 6179.See §34.8.Ernst, F.J., García D., A. and Hauser, I. (1987). Colliding gravitational plane waveswith noncollinear polarization.I.JMP 28, 2155.See §§25.2, 25.4, 25.5.Ernst, F.J., García D., A. and Hauser, I. (1988). Colliding gravitational plane waveswith noncollinear polarization.III.JMP 29, 681.See §§25.4, 25.5, 34.6.Ernst, F.J. and Wild, W.J. (1976). Kerr black holes in a magnetic universe. JMP 17,182.See §§21.1, 34.1.Estabrook, F.B. (1976). Some old and new techniques for the practical use of exteriordifferential forms, in Bäcklund transformations.Lecture notes in mathematics,vol.515, ed.R.M.Miura, page 136 (Springer Verlag, Berlin).See §10.4.Estabrook, F.B. (1982). Moving frames and prolongation algebras. JMP 23, 2071.See §10.4.Estabrook, F.B. and Wahlquist, H.D. (1976). Prolongation structures of nonlinearevolution equations II.JMP 17, 1293.See §10.4.Estabrook, F.B., Wahlquist, H.D. and Behr, C.G. (1968). Dyadic analysis of spatiallyhomogeneous world models.JMP 9, 497.See §8.2.Evans, A.B. (1977).Static fluid cylinders in general relativity. J. Phys. A 10, 1303.See§22.2.Fackerell, E.D. and Kerr, R.P. (1991). Einstein vacuum field equations with a singlenon-null Killing vector.GRG 23, 861.See §17.3.Faridi, A.M. (1990). Einstein–Maxwell equations and the groups of homothetic motion.JMP 31, 401.See §11.3.Farnsworth, D.L. (1967). Some new general relativistic dust metrics possessingisometries.JMP 8, 2315.See §14.3.Farnsworth, D.L. and Kerr, R.P. (1966). Homogeneous dust-filled cosmologicalsolutions.JMP 7, 1625.See §§8.2, 12.4.Fee, G.J. (1979). Homogeneous spacetimes. M. Math. thesis, University of Waterloo.See §12.1.Feinstein, A.and Griffiths, J.B.(1994).Colliding gravitational waves in a closedFriedmann–Robertson–Walker background.CQG 11, L109.See §25.6.Feinstein, A.and Ibañez, J.(1989).Curvature-singularity-free solutions for collidingplane gravitational waves with broken u − v symmetry. PRD 39, 470.See §25.3.Feinstein, A., MacCallum, M.A.H. and Senovilla, J.M.M. (1989). On the ambiguousevolution and the production of matter in spacetimes with colliding waves. CQG6, L217.See §25.6.Feinstein, A. and Senovilla, J.M.M. (1989a). Collision between variably polarized planegravitational wave and a shell of null matter.Phys. Lett. A 138, 102.See §25.6.Feinstein, A. and Senovilla, J.M.M. (1989b). A new inhomogeneous cosmologicalperfect fluid solution with p = ρ/3.CQG 6, L89.See §23.3.Fels, M.and Held, A.(1989).Kerr–Schild rides again.GRG 21, 61.See §§29.2, 32.5.Fernandez-Jambrina, L.(1994).Moment density of Zipoy’s dipole solution.CQG 11,1483.See §20.2.Fernandez-Jambrina, L.(1997).Singularity-free cylindrical cosmological model.CQG14, 3407.See §23.3.