Contents

638 ReferencesGarcía D., A. and Breton B., N. (1985). The gravitational field of a charged,magnetized, accelerating, and rotating mass.JMP 26, 465.See §34.1.García D., A. and Breton B., N. (1989). Magnetic generalizations of the Carter metrics.JMP 30, 1310.See §34.1.García D., A. and Hauser, I. (1988). Type-D rigidly rotating perfect fluid solutions.JMP 29, 175.See §21.2.García D., A.and Kramer, D.(1997).Stationary cylindrically symmetric gravitationalfields with differentially rotating perfect fluids.CQG 14, 499.See §22.2.García D., A.and Macias, A.(1998).Black holes as exact solutions of the Einstein–Maxwell equations of Petrov type D, inBlack holes: Theory and observation.Lecture notes in physics, vol. 514, eds. F.W. Hehl, C. Kiefer and R.J.K. Metzler,page 205 (Springer, Berlin).See §21.1.García D., A. and Plebański, J.F. (1981). All nontwisting N’s with cosmologicalconstant.JMP 22, 2655.See §§28.4, 31.8.García D., A. and Plebański, J.F. (1982a). An exceptional type D shearing twistingelectrovac with Λ.JMP 23, 123.See §26.1.García D., A. and Plebański, J.F. (1982b). Solutions of type D possessing a groupwith null orbits as contractions of the seven-parameter solution. JMP 23, 1463.See §24.3.García D., A. and Salazar I., H. (1983).All null orbit type D electrovac solutions withcosmological constant.JMP 24, 2498.See §24.3.Gardner, R.B. (1989). The method of equivalence and its applications (SIAM,Philadelphia).See §§7.4, 9.2.Garfinkle, D. (1991).Cosmic-string traveling waves, in Nonlinear problems in relativityand cosmology, eds. J.R. Buchler, S.L. Detweiler and J.R. Ipser, page 68(New York Acad.Sci, New York, NY).See §32.5.Garfinkle, D., Glass, E.N. and Krisch, J.P. (1997). Solution generating with perfectfluids.GRG 29, 467.See §17.3.Garfinkle, D.and Melvin, M.A.(1994).Generalized magnetic universe solutions.PRD50, 3859.See §34.1.Garfinkle, D.and Tian, Q.(1987).Spacetimes with cosmological constant and aconformal Killing field have constant curvature.CQG 4, 137.See §35.4.Gautreau, R.and Hoffman, R.B.(1972).Generating potential for the NUT metric ingeneral relativity.Phys. Lett. A 39, 75.See §20.3.Gautreau, R.and Hoffman, R.B.(1973).The structure of the sources of Weyl-typeelectrovac fields in general relativity.Nuovo Cim. B 16, 162.See §18.6.Gautreau, R., Hoffman, R.B. and Armenti, A. (1972). Static multiparticle systems ingeneral relativity.Nuovo Cim. B 7, 71.See §21.1.Gavrilina, G.A. (1983). Generalized Kerr–Schild space-times with null Killing vectors,in 10th international conference on general relativity and gravitation, vol.1.Contributed papers. Classical relativity, eds.B.Bertotti, F.De Felice and A.Pascolini, page 233 (Consiglio Nazionale delle Ricerche, Rome).See §32.5.Géhéniau, J.(1957).Une classification des espaces einsteiniens.C. R. Acad. Sci.(Paris) 244, 723.See Ch.4.Gergely, L.A. and Perjés, Z.(1993).Solution of the vacuum Kerr–Schild problem.Phys. Lett. A 181, 345.See §32.5.Gergely, L.A. and Perjés, Z.(1994a).Kerr–Schild metrics revisited.I.The groundstate.JMP 35, 2438.See §32.5.Gergely, L.A. and Perjés, Z.(1994b).Kerr–Schild metrics revisited.II.The completevacuum solution.JMP 35, 2448.See §32.5.Gergely, L.A. and Perjés, Z.(1994c).Vacuum Kerr–Schild metrics generated bynontwisting congruences.Ann. Phys. (Germany) 3, 609.See §32.5.Geroch, R.(1969).Limits of spacetimes.Commun. Math. Phys. 13, 180.See §9.5.Geroch, R.(1970a).Multipole moments.I.Flat space.JMP 11, 1955.See §18.8.