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Точные решения уравнений Эйнщтейна - Крамер Д.

Крамер Д., Штефани Э., Херльт М., Мак-Каллум М. Точные решения уравнений Эйнщтейна — М.: Энергоиздат, 1982. — 416 c.
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381
Ehlers, J. (1961). BeUrage гиг relatitislischen Xeehanik JcotUinuierlteher Лfedien, Akad. Win.

Lit. Mainz, Abhandl. Math.-Nat. Kl., Kr. 11. See §§ 6.1., 33.1,

Ehlers, J. (1962). TrantformtUione of static exterior solutions of Einstein's gravitational field equations into different solutions by means of conformed mappings, ColIoques International»* C.N.R.S. No. 91 (Les theories relativistes de la gravitation), 276. See §§ 19.2., 30.6.

'Ehlers, J. See also Jordan et al. (I960, 1961)

Ehlers, J., and Kundt, W. (1962). Exact solutions of the gravitational field equations, in: Witten, L. (Ed.), Gravitation: an introduction to current research, Wiley, New York, London. See §§ 1.4., 6.1., 6.1., 16.6., 21.5., 31.1.. 31.2.

Ehlers, J., Kosenblum, A., Goldberg, J. N., and Havas, P. (1976). Comments on gravitational radiation damping and energy loss in binary systems, Astrophvs. J. 208, L. 77. See § 1.1. Einstein, A., and Rosen, N. J. (1937). On gravitational waves, J. Franklin Inst. 228, 43. See § 20.3.

Einstein, A., and de Sitter, W. (1932). On the relation between the expansion and mean velocity of the universe, Proc. Natl. Acad. Sci. U.S. IS, 213. See § 12.2.

Eisenhart, L. P. (1933). Continuous Groups of Transformations, Princeton Univ. Press.'See §§ 8.1., 8.4., 8.5.,8.6.

Eisenhart, L. P. (1949). Riemannian Geometry, Princeton Univ. Press. See §§3.1., 3.7., 8.4.,

31.1., 32.1.. 32.3.

Ellis. G. F. R. (1967). Dynamics of pressure-free matter in general relativity, J. Math. Phys. 8, 1171. See §§9.2., 11.1., 11.4., 13.5.

Ellis, G. F. R. See also Hawfcing and Ellis (1973), King and Ellis (1973), Stewart and Bllis (1968) Ellis, G. R. F. and King, A. R. (1974). ITim the big bang a whimperl Commun. Math. Phvs. 88. 119. See § 12.1.

Ellis, G. F. R., and MacCallum, M. A. H., (1969). A class of homogeneous cosmological models, Commun. Math. Phys. 12, 108. See §§8.2., 11.2., 11.3., 12.4.

Eltgroth, P. G. See Vajk and Eltgroth (1970)

Ernst. F. J. (1968a). New formulation of the axially symmetric gravitational field problem.

Phys. Rev. 167, 1175. See §§ 17.5., 18.5.

Ernst, F. J. (1968b). New formulation of the axially symmetric gravitational field ргоЫет II.

Phys. Rev. 168, 1415. See § 16.4.

Ernst, F. J. (1973). Charged version of Tomimatsu-Sato spinning mass field, Phys. Rev. D ", 2520. See § 30.6.

Ernstt1F. J. (1976a). Removal of the nodal singularity of the C-nutric, J. Math. Phys. 17, SIS. See § 191.

Ernst, F. J. (1976b). New representation of the Tomimatsu-Sato solution, J. Math. Phys. 17, 1091. See § 18.5.

Ernst, F. J. (1977). A new family of solutions of the Einstein field equations, J. Math. Phys. 18. 233. See § 18.6.

Ernst, F. J. (1978). Coping with different languages in the null Mrad formulation of general relativity, J. Math. Phys. 19, 489. See § 7.1.

Ernst. F. J. See also Hauser and Ernst (1978a, b)

Ernst, F. J.. and Hauser, I. (1978). Field equations and integrabUity conditions for special type N twisting gravitational fields, J. Math. Phys. 19, 1816. See § 25.3.

Ernst, J. F., and Wild, W. J. (1976). Kerr black holes in a magnetic universe, J. Math. Phvs.

17, 182. See § 30.5.

Esposito, F. P., and Glass, E. N. (1976). The Weyl tensor and stationary electrovac space-times.

J. Math. Phys. 17, 282. See § 16.6.

Esposito, F. P., and Witten, L. (1973). Five-parameter exterior solution of the Einstein-Maxinll field equations, Phys. Rev. D 8, 3302. See § 30.5. brook, F. B. See WahIquist and Estabrook (1966)

Estabrook, F. B., Wahlqiiist, H. D., nnd Behr, C. G. (1968). Dyadic analysis of spatially homogeneous world models, J. Math. Phys. 9, 497. See §8.2.

Evans, A. B. (1977). Static fluid cylinders in general relativity, J. Phys. A 10, 1303. See § 20.2. Evans, A. B. (1978). Correlation of Neirtonian and relativistic cosmoiog/f, Mon. Not. Roy.

Astr. Soc. 183, 727. See §§ 11.3., 12.4.

Exton, E. See Newman et al. (1966)

Farnsworth, D. L. (1967). Some new general relativistic dust metrics pntessing isometrics. J 1 Math. Phys. 8, 2315. See § 12.3.

382
Fa г па worth, D. L., and Kerrt R. P. (1966). Homogenrous dust-filled cosmological *ЫиИоп*„ J. Math. Phys. 7, 1625. See §§ 8.2., 10.4.

Finkelstein, D. (1958). Paat future asymmetry of the gravitational field of a point particle. Phys*.

Rev. HO, 965. See § 13.4.

Finkelstein, R. J. (1975). The general relativistic fields of a charged rotating source, J. Matlu -Phys. їв, 1271. See $30.6.

Klahertvt E. J. See Cox and T4Iaherty (1976)

Flanders, H. (1963). Differential Forms with Application* to the Physical Sciencesy Arad* Press, New York. See §§ 2.1., 2.7.

Kostert J., and Newmant E. T. (1967). Note on the Robinson-Trauiman Solutiongi J. Math.

Phvs. 8» 189. Set § 24.1.

Foystcr, J. M. See McIntosh and Foyeter (1972)

Foyetert J. M. and McIntosh» C. B. 0. (1972). A class of solutions of Einstein's equations which admit a З-parameter group of tsomelries, Commun. Math. Phys. 27, 241. See $ 13.4. Franraviglia, M. Sec Benenti and Francaviglin (1979)
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