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References 659Lesame, W.M., Ellis, G.F.R. and Dunsby, P.K.S. (1996). Irrotational dust withdivH =0.PRD 53, 738.See §§6.2, 23.3.Letelier, P.S. (1975). Self-gravitating fluids with cylindrical symmetry. JMP 16, 1488.See §10.11.Letelier, P.S. (1979). Self-gravitating fluids with cylindrical symmetry. II. JMP 20,2078.See §10.11.Letelier, P.S. (1982). New two-soliton solution to the Einstein equations. PRD 26,3728.See §34.5.Letelier, P.S. (1985a). On the superposition of stationary axially symmetric solutionsto the vacuum Einstein equations.CQG 2, 419.See §34.5.Letelier, P.S. (1985b). Solitary wave solutions to the Einstein equations. JMP 26, 326.See §34.5.Letelier, P.S. (1985c). Static and stationary multiple soliton solutions to the Einsteinequations.JMP 26, 467.See §34.5.Letelier, P.S. (1986). Soliton solutions to the vacuum Einstein equations obtained froma nondiagonal seed solution.JMP 27, 564.See §34.5.Letelier, P.S. and Oliveira, S.R. (1988). Superposition of Weyl solutions to the Einsteinequations: cosmic strings and domain walls.CQG 5, L47.See §20.2.Letelier, P.S. and Oliveira, S.R. (1998a). Double Kerr–NUT spacetimes: spinningstrings and spinning rods.Phys. Lett. A 57, 6113.See §34.5.Letelier, P.S.and Oliveira, S.R.(1998b). Superposition of Weyl solutions: theequilibrium forces.CQG 15, 421.See §20.2.Letelier, P.S. and Tabensky, R.R. (1974). The general solution to Einstein–Maxwellequations with plane symmetry.JMP 15, 594.See §15.4.Letelier, P.S. and Tabensky, R.R. (1975). Cylindrical self-gravitating fluids withpressure equal to energy density.Nuovo Cim. B 28, 407.See §10.11.Letelier, P.S. and Wang, A. (1993). On the interaction of null fluids in cosmology. Phys.Lett. A 182, 220.See §25.6.Letniowski, F.W. and McLenaghan, R.G. (1988). An improved algorithm forquartic equation classification and Petrov classification. GRG 20, 463. See§9.3.Levi-Civita, T.(1917a).ds 2 einsteiniani in campi newtoniani. Rend. Acc. Lincei 27,183.See §§18.6, 22.2.Levi-Civita, T.(1917b).Realtá fisica di alcuni spazi normali del Bianchi. Rend. R.Acad. Lincei, Cl. Sci. Fis. Mat. Nat. 26, 519.See §12.3.Lewandowski, J.(1990).Conformal symmetries of pure radiation.CQG 7, L135. See§35.4.Lewandowski, J.(1992).Reduced holonomy group and Einstein equations with acosmological constant.CQG 9, L147.See §31.8.Lewandowski, J.and Nurowski, P.(1990).Algebraically special twisting gravitationalfields and CR structures.CQG 7, 309.See §30.7.Lewandowski, J., Nurowski, P. and Tafel, J. (1991). Algebraically special solutions ofthe Einstein equations with pure radiation fields.CQG 8, 493.See §30.7.Lewis, T.(1932).Some special solutions of the equations of axially symmetricgravitational fields.Proc. Roy. Soc. Lond. A 136, 176.See §§19.3, 20.4.Li, Jian-Zeng and Liang, Can-Bin (1989).Static ‘semi-plane-symmetric’ metricsyielded by plane-symmetric electromagnetic fields.JMP 30, 2915.See §22.2.Li, W.(1988).The complete Virasoro algebra for the stationary and axially symmetricEinstein field equations.Phys. Lett. A 129, 301.See §34.7.Li, W.(1989a).Generalization of the Hauser–Ernst formalism for two-dimensionalreduced Einstein abelian gauge field equations. Phys. Lett. A 134, 343. See§34.7.Li, W.(1989b).New families of colliding gravitational plane waves with collinearpolarisation.CQG 6, 477.See §25.4.

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