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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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Hauser, I., and Malhiot, R. J. (1974). Spherically symmetric Itatic space-times v.-hirh admit stationary Killing tensors of rank two, J. Math. Phys. 15, 816. See § 31.3.

Hauser, I., and Malhiot, R. J. (1975). Structural equations for Killing tensors of onler tiro.

I, 11, J. Math. Phys. 16, 150, 1625. See § 31.3.

Hauser, I., and Malhiot, R. J. (1976). On space-time Killing tensors vrith a Segri characteristic

[(11) (11)], 3. Math. Phys. 17, 1306. See § 31.3.

Hauser, I., and Malhiot, R. J. (1978). Forms of all space-time metrics which admit [(11)(11)1

Killing tensors with nonconstant eigenvalues, J. Math. Phys. 19, 187. See § 31.3.

Havas, P. (1975). Separation of variables in the Hamilton-Jacobi. Schrndinger, and relate? equations. 1, 11, 3. Math. Phys. 10. 1461. 2476. See § 31.3.

Havas, P. See also Ehlere et al. (1976)

Hawking, S. W. See Hartle and Hawking (1972)

Hawking, S. W., and Ellis, G. F. R. (1973). The large scale structure of space-time, Cambridge Univ. Press. See §§ 2.1., 5.3., 10.4.

Heintzmann, H. (1969). New exact static solutions of Einstein's field equations, Z. Phys. 22$, 489. See § 14.1.

Held, A. (1974 a). A type-(3,1) solution to the vacuum Einstein equations, N. Cim. Lett. 11, 545. See §§ 25.2., 25.4.

25—99

385
Held, Л. (1974b). A formalism for th< inCfMiffation of algebraically special metrics. I, Commuti Math. Phys. 37, 311. See § 7.3.

Held, A. (1975). A formalism for the investigation of ulgebrnically special metrics. II, Common.

Math. Phys. 44, 211. Set § 7.3.

Held, A. (1976a). Killing vectors in empty space algfbrnlcally special metrics. I, GPvG 7, 177. See §§ 7.3., 26.4., 33.2.

Held, A. (1976b). Killing vectors in empty space algebraically special metrics. II, J. Math.

Phys. 17, 39. See 33.2.

Held, A. See also Geroch et al. (1973)

Helga3on. S. (1962). Differential Geometry and Symmetric Spaces, Acad. Press, New York. See § 2.1.

Herlt. E. (1972). Dber eine Klasse innerer stationarer axial-symmetrischer Liisungen der Einstein• schen FeldgleicAungen mil idealem fIuiJem Medium, Wis?. Z. Uiiir. Jena, Math.-Nat, R. SI, 19. See $ 19.2.

Heilt, E. (1978). Static and stationary axially symmetric gravitational fields of bounded sources.

I. Sciulions obtainable from the van Stockum metric, GBG #, 711, See §§ 19.1., 30.3., 30.5. Herlt, E. (1979). Static and stationary axially symmetric gravitational fields of bounded sources.

II. Solvtions obtainable from WeyVs class, GBG 11, 337. See § 19.1.

Hiromoto, R. E., and Ozsvath, I. (1978). On homogeneous solutions of Einsteins field equations.

URG », 299. See §§ 10.1., 10.2.

Hoenselaers. C. (1976). On generation of solutions of Einstein's equations, J. Math. Phys. 17. 1264. See § 30.2.

Hoenscloerst C. (1978a). A new solution of Ernst’s equation, J. Phys. AU, L75. See § 18.6. Hoenselaerg, C. (1978 b). On the effect of motions on energy-momentum tensor, Prog. Theor.

Phys. 59,1518. See $ 9.1.

Hoensetaers, C. (1978c). Algtbraically special one Killing vector solutions of Einstein's equations, Prog. Theor. Phys. 60, 747. See § 15.4.

Hoenselaers, C., and Vishveshwara, С. V. (1979). Interiors with relativistic dust-flow, J. Phys. A 12, 209. See $ 19.2.

Hoffman, R. B. (1969a). Stationary axially symmetric generalizations of the Weyl solution in general relativity, Phys. Rev. 182,1361. See § 18.4.

Hoffman, R. B. (1969b). Stationary *noncanonieal’ solutions of the Einstein vacuum field equations, 3. Math. Phys. 1Ф, 953. See $ 21.5.

Hoffman, R. B. See also Gautreau and Hoffman (1970, 1972, 1973), Ciautreau et al. (1972) Hori, S. (1978) On the exact solution of Tomimatsu-Sato family for an arbitrary integral value of the deformation parameter, Prog. Theor. Phys. 59, 1870. See § 18.5.

Horsky, J. (1975). The gravitational field of a homogeneous plate with a non-zero cosmological constant, Czech. J. Phys. B 25, 1081. See § 13.6.

Horsky, J. See also Novotny and Horsky (1974), Avakyan and Horaky (1975)

Horsky. J., and Novotny, J. (1972). The generalized Taub solution, Bull. Astiron. Inst. Czech. 28, 266. See $ 12.4.

Horsky, J., Lorenc, P., and Novotny, J. (1977). A non-static source of the Taub solution of Einstein’s gravitational equations, Phys. Letters A 63, 79. See $ 13.5.

Hughston, L. P. (1971). Generalized Vaidya metrics, Int. J. Theor. Phys. 4, 267. See § 26.6. Hughston, L. P., and Sommers, P. (1973). Spacetimes with Killing tensors, Commun. Math.

Phys. 82, 147. See § 31.3.

Hughston, L. P., Penrose, R., Sommers, P., and Walker, M. (1972). On a quadratic first integral for the charged particle orbits in the charged Kerr solution, Commun. Math. Phys. 27, 303. See §31.3.

Ihrig, E. (1975). The uniqueness of gtf in terms of Int. J. Theor. Phys. 14. 23. See § 31.4. Ikeda, M., Kitamura1 S., and Matsumoto, M. (1963). On the embedding of spherically symmetric space-times, 3. MaUu Kyoto Univ. 8, 71. See § 32.3.

Israel, W. (1958). Discontinuities in spherically symmetric gravitational fields and shells of radiation, Proc. Roy. Soc. Lond. A 248, 404. See § 13.1.
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