Точные решения уравнений Эйнщтейна - Крамер Д.
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Frchland. K. (1972). Kxact gravitational field of the infinitely long rotating hollow cylinder*.
(’oiiirmm. Math. Phvs. 20. 307. Sre §20.2.
French. I). <\ .Vrr (‘ollinson and French (1967)
Friedman. А. (19651. Isotuefr Ir, embedding of Fiemayiniun muni folds into euclidean space*.
Rev Mod. Phys. 37. 201. See. §$32.3.. 32.7.
Friedmann. Л. (1922). Cber die Kriimmung des Bauniest Z. Phys. 10, 377. See. $ 12.2. Friedmann, A. (1924). Ober die M<*jlichkeit einer Welt mit konst ante r nrgaticer Kriimmung dcs Raumest Z. Phys. 21, 326. See $ 12.2.
Frolov, V. P. (1974). Kerr anil NevymaH-Vnti-Tamhurino type solutions of Kinstein'-* equation* with cosmological term (in Russian), Teor. Mat. Fiz. 21, 213. See. § 18.5.
Frolov, V. P., and Khlebnikov, V. I. (1975). Gravitational field of radiating system* I. Twisting free type Jt metric*. Preprint no. 27, Lebedev Phvs. [nst., Akad. Xauk, Moscou . AVf $24.3. Frolov, V. P. (1977). Xewman-Penrose formalism in general relativity (in Russian), Problems in GeneraI Relativity and Theory of Group Representations, Trudv Lebedev Inst.. Akad. Xauk SSR, 96. 72- 180. .See §§ 7?., 24.1.
Fnmsdal. C. (1959). (’ompletion and embedding of the Schunrzschild solution, Phys. Rev. IHL 778. See $32.7.
Fugm4, J. See Collinson and" Fugerc (1977)
Gatitrcau, R.. and Hoffman, R. B. (1970). Class of exact solution of the Kinsirin-NnxutTlf it/nations. Phys. Rev. I) 2, 271. See § 30.5.
< .\iutie.ni, R., and Hoffman, R, B. (1972). Generating potential for the ХГТ imtric in general
relativity, Phys. Letters Л 39, 75. See § 18.3.
Gautreau, R.* and Hoffman, R. B. (1973). The structure of the sources of Weyl-type electronic
fields in general relativity, N. Cim. B 16, 162. See § 16.6.
Gautieau, R., Hoffman, R. B., and Armenti. A. (1972). Static multi particle system* in grnerat relativity, N. Cim. B 7, 71. AVe $ 19.1,
Geheninu, «I. (1956). Les invariants de courbure des espaces riemunnirns de In relatiritr. Hull.
Acad. Roy. Belgique* Cl- Sci. 42, 253. See § 5.1.
Gehi-Iiiau, J. (1957). Vne classification des espaces einsteiniens C.R. Arad. Sci. (IVuis) 244,
723. See І 4.3.
< !('¦Іи-шаи. J., and Debever, R. (1956a). Lrs quatorze invariants de. rourburr dr. Vrspttcr cirwannien
a qu/itre dimensions, Helv. Phys. Acta. Stippl. 4, 101. AVe $ 31.4.
G6heiiiau, J.( and Debever, R. (1956b). Les invariants dr. courbure de Vespaa '/• Hirmttun
а qtuitre. dimensions. Bull. Acad. Koy. Belgique Cl. «Sci. 42, 114. See § 5.1.
t 'eroeh. R. (I960). Limits of spacetimes, ('ommuii. Math. Phys. 13, ISO. See § 30.0.
(Serochf R. (1971). .4 method for generating solutions of Kinsteins eqtuition.'*. J. Math. Phys.
12. 918. See $§ 16.1., 30.3.
Gprocha R. (1972), A method for generating new solutions of Einstein’s equation. I/. J. Math.
Phys. J3, 394. AVe §§ 17.3L, 30.4.
(Seroch, R., Held, A., and Penrose, R. (1973). .4 space-time calculus based on pairs of null
directions. J. Math. Phys. 14, 874. See $ 7.3. tibbons, 0* W.. and Russell-Clark, R. A. (1973). Note on the. Sato-Tomimatsu solution af
J'CinsUvn11 equations» Phys. Rev. Lett. 30, 398. See § 18.5.
383-
<і!й85. К. N. (1U7">). The Weyl tensor and shear-free -perfect fluids, J. Mnth. Phys. 16, 2361. Л'се SS 0.2., 16.0.
\Sloss, E N. Ser also Collins et al. (1980), EspoRito and Glass (1976)
Glass, E. ГГ., and Goldman, S. P. (1978). Relativistic spherical stars reformulated, J. Math. Phys. 1», 856. See $ 14.1.
Code!, K. (1949). .4» example of a new type of cosmological solution of Einstein's field equation of gravitation. Rev. Mod. Phys. 21, 447. See § 10.4.
GoeL P. See Guptn and (Joel (1975)
<«oenner, H. (1970). Einstein tensor and generalizations of Birkhoff's theorem. l .^r";iun. Math. Phys. 16, 34. See § 13.4.
Goenncr, H. (1973). Local isometric embedding of Riemannian manifolds and Einstein’s theory of gravitation, Habilitationsschrift, Gottingen. See §§ 32.3., 32.5.
Gocnner, H. (1977). On the interdependence of the Oavss-Codazzi-Ricci equations of local isometric embedding, GRG 8, 139. See SS 32.2., 32.4.
Goenner, H. (1980). Local isometric embedding of Riemannian manifolds and Einstein's theory of gravitation, in Held, A. (Ed.), General Relativity and Gravitation one hundred years after the birth of Albert Einstein, Vol. I, Plenum Press, New York. See § 32.1.
Goenner, H., and Stachel, J. (1970). Einstein tensor and З-parameter groups of isometries with 2-dimensional orbits. J. Math. Phys. 11, ЗЗЛЯ. See §jj 13.1., 13.2., 13.4.
Goldberg, J. N. See Ehlers et al. (1976), Kerr and (Joldberg (1961)
Goldberg, J. N., and Kerr, R. P. (1961). Some ajrplicalions of the. infinitesimal holonomy group to the Petrov classification of Einstein spaces, J. Math. Phys. 2, 327. See § 31.4.
Goldberg, J. N., and Sachs, R. K. (1962). A theorem on Petrov types, Acta Phys. Polon., Suppl. 22.13. See S 7-5.
Goldman, S. P. See Glass and Goldman (1978)
-Goodinson, P. A. (1969). The electromagnetic tensor in Riemannian space-time, Anales de Fisica 65, 351. See § 0.2.
