Contents

618 ReferencesBasu, A., Ganguly, S. and Ray, D. (1990). Perfect fluid in a static isotropic universe.Int. J. Theor. Phys. 29, 435.See §18.6.Batakis, N.and Cohen, J.M.(1972).Closed anisotropic cosmological models.Ann.Phys. (USA) 73, 578.See §14.3.Bayin, S.S. (1978). Solutions of Einstein’s field equations for static fluid spheres. PRD18, 2745.See §16.1.Bayin, S.S. and Krisch, J.P. (1986). Fluid sources for Bianchi I and III space-times.JMP 27, 262.See §14.3.Beck, G.(1925).Zur Theorie binärer Gravitationsf elder.Z. Phys. 33, 713.See §22.3.Beig, R.and Simon, W.(1980).Proof of a multipole conjecture due to Geroch.Commun.Math. Phys. 78, 75.See §18.8.Beig, R.and Simon, W.(1981).On the multipole expansion for stationary space-times.Proc. Roy. Soc. London A 376, 333.See §18.8.Beiglböck, W.(1964).Zur Theorie der infinitesimalen Holonomiegruppe in der AllgemeinenRelativitätstheorie.Z. Phys. 179, 148.See §9.1.Bel, L.(1959).Quelques remarques sur la classification de Petrov.C. R. Acad. Sci.(Paris) 248, 2561.See Ch.4.Belinski, V.A. and Verdaguer, E. (2001).Gravitational solitons (Cambridge UniversityPress, Cambridge).See §1.4, Ch. 23, §34.5.Belinskii, V.(1979).Single-soliton cosmological waves.Zh. Eks. Teor. Fiz. 77, 1239. See§10.11.Belinskii, V.and Fargion, D.(1980a).The inverse scattering method in the theory ofgravitation.Rend. Sem. Mat. Univ. Politec. Torino 38, 1.See §10.11.Belinskii, V.and Fargion, D.(1980b).Two-soliton waves in anisotropic cosmology.Nuovo Cim. B 59, 143.See §34.5.Belinskii, V.and Francaviglia, M.(1982).Solitonic gravitational waves in Bianchi IIcosmologies.I.The general framework.GRG 14, 213.See §34.5.Belinskii, V.and Francaviglia, M.(1984).Solitonic gravitational waves in Bianchi IIcosmologies.II.One solitonic perturbations.GRG 16, 1189.See §34.5.Belinskii, V.and Zakharov, V.E.(1978).Integration of the Einstein equations by theinverse scattering problem technique and the calculation of the exact soliton solutions.Sov.Phys. JETP 75, 1953.See §§22.3, 34.5, 34.6.Belinskii, V.A. and Zakharov, V.E. (1979).Stationary gravitational solitons with axialsymmetry.Sov. Phys. JETP 77, 3.See §34.5.Bell, P.and Szekeres, P.(1972).Some properties of higher spin rest-mass zero fields ingeneral relativity.Int. J. Theor. Phys. 6, 111.See §§7.3, 7.6.Bell, P.and Szekeres, P.(1974).Interacting electromagnetic shock waves in generalrelativity.GRG 5, 275.See §25.5.Benenti, S.(1997).Intrinsic characterization of the variable separation in the Hamilton–Jacobi equation.JMP 28, 6578.See §35.3.Benoit, P.M. and Coley, A.A. (1998).Spherically symmetric spacetimes and kinematicself-similarity.CQG 15, 2397.See §35.4.Berger, B.K., Eardley, D. and Olson, D.W. (1977). Note on the spacetimes of Szekeres.PRD 16, 3086.See §§36.2, 36.3.Bergmann, P.G., Cahen, M. and Komar, A.B. (1965). Spherically symmetric gravitationalfields.JMP 6, 1.See §15.4.Bergstrom, L.and Goobar, A.(1999).Cosmology and particle astrophysics (Praxis andJohn Wiley and Sons, Chichester).See §14.1.Bertotti, B.(1959).Uniform electromagnetic field in the theory of general relativity.Phys. Rev. 116, 1331.See §§12.3, 21.1.Bhatt, P.V. and Vaidya, S.K. (1991). Kerr–Schild type solutions of Einstein–Maxwellequations.CQG 8, 1717.See §32.5.Bhutani, O.P.and Singh, K.(1998).Generalized similarity solutions for the type Dfluid in five-dimensional flat space.JMP 39, 3203.See §37.4.