Contents

668 ReferencesNeugebauer, G.and Meinel, R.(1993).The Einsteinian gravitational field of the rigidlyrotating disk of dust.Astrophys. J., Lett. 414, L97.See §34.6.Neugebauer, G.and Meinel, R.(1994).General relativistic gravitational field of arigidly rotating disk of dust: axis potential, disk metric, and surface mass density.Phys. Rev. Lett. 73, 2166.See §34.6.Neugebauer, G.and Meinel, R.(1995).General relativistic gravitational field of arigidly rotating disk of dust: Solution in terms of ultraelliptic functions. Phys.Rev. Lett. 75, 3046.See §§21.2, 34.6.Newman, E.T., Couch, E., Chinnapared, K., Exton, A., Prakash, A. and Torrence,R.J. (1965).Metric of a rotating charged mass.JMP 6, 918.See §§21.1, 32.3.Newman, E.T. and Janis, A.I. (1965). Note on the Kerr spinning-particle metric. JMP6, 915.See §21.1.Newman, E.T. and Penrose, R. (1962). An approach to gravitational radiation by amethod of spin coefficients.JMP 3, 566.See §§7.1, 7.2, 7.6.Newman, E.T. and Tamburino, L.A. (1962). Empty space metrics containinghypersurface orthogonal geodesic rays.JMP 3, 902.See §26.4.Newman, E.T., Tamburino, L.A. and Unti, T. (1963). Empty-space generalization ofthe Schwarzschild metric.JMP 4, 915.See §§13.3, 29.5.Newman, E.T. and Unti, T.W.J. (1963). A class of null flat-space coordinate systems.JMP 4, 1467.See §§28.3, 32.1.Nilsson, U.S.and Uggla, C.(1997a).Rigidly rotating stationary cylindrically symmetricperfect fluid models.CQG 14, 2931.See §22.2.Nilsson, U.S. and Uggla, C. (1997b). Stationary Bianchi type II perfect fluid models.JMP 38, 2616.See §13.4.Nordström, G.(1918).On the energy of the gravitational field in Einstein’s theory.Proc. Kon. Ned. Akad. Wet. 20, 1238.See §§15.4, 21.1.Novikov, I.D. (1963). On the evolution of a semiclosed universe (in Russian). Zh.Astrof. 40, 772.See §15.4.Novikov, I.D. (1964). R- and T-regions in a spacetime with a spherically symmetricspace (in Russian).Comm. State Sternberg Astron. Inst. 132, 3.See §14.3.Novotný, J.and Horský, J.(1974).On the plane gravitational condensor with thepositive gravitational constant.Czech. J. Phys. B 24, 718.See §15.4.Nurowski, P., Hughston, L.P. and Robinson, D.C. (1999). Extensions of bundles of nulldirections.CQG 16, 255.See §9.4.Nurowski, P.and Robinson, D.C.(2000).Intrinsic geometry of a null hypersurface.CQG 17, 4065.See §9.4.Nurowski, P.and Tafel, J.(1992).New algebraically special solutions of the Einstein–Maxwell equations.CQG 9, 2069.See §30.5.Nutku, Y.(1991).Spherical shock waves in general relativity.PRD 44, 3164. See§28.1.Nutku, Y.and Halil, M.(1977).Colliding impulsive gravitational waves.Phys. Rev.Lett. 39, 1379.See §25.4.O’Brien, S.and Synge, J.L.(1952).Jump conditions at discontinuities in generalrelativity.Comm. Dublin Inst. Advanced Studies A 9, 1.See §3.8.Öktem, F.(1976).On parallel null 1-planes in space-time.Nuovo Cim. B 34, 169. See§6.1.Oleson, M.(1971).A class of type [4] perfect fluid space-times.JMP 12, 666. See§33.4.Oleson, M.(1972).Algebraically special fluid space-times with shearing rays.Ph.D.thesis, University of Waterloo.See §§33.1, 33.4.Oliver, G.and Verdaguer, E.(1989).A family of inhomogeneous cosmologicalEinstein–Rosen metrics.JMP 30, 442.See §§10.11, 34.5.Olver, P.J. (1986).Applications of Lie groups to differential equations.Graduate Textsin Mathematics, vol.107 (Springer-Verlag, Berlin).See §10.2.