Точные решения уравнений Эйнщтейна - Крамер Д.
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Letelier1 P. S., and Tabensky, R. R. (1975b). Singularities for fluids with jp = to equations of state, JT. Math. Phys. 16, 8. See $ 20.5.
Levi-Civita, T. (1917—1919). ds* einsteiniani in campi newtoniani, Rend. Acc. Lincei 86, 307 (1917), 27, 3,183, 220, 240,283,343 (1918), 28, 3,101 (1919). See §§ 16.6., 20.2.
Levine, J. (1936). Groups of motions in conformally flat spaces. I, Bull. Amcr. Math. Soc. 42, 418. See § 22.2.
Levine, J. (1939). Groups of motions in conformally flat spaces. II, Bull. Amer. Math. Soc. 45, 766. See § 22.2.
Levine, J. See also Katzin and Levine (1972), Kutzin et al. (1969)
Levy, H. (1968). Classification, of stationary axisymmetric gravitational fields, N. Сію. B 68, 253. See § 18.4.
Lewis, T. (1932). Some special solutions of the equations of axially symmetric gravitational fields, Proc. Roy. Soc. Lond. A 186, 176. See §§ 17.3., 18.4.
Liohnerowicz1 A. (1955). Thiories relativistes de la gravitation et de Vilectromagnitisme, Masson, Paris. See § 16.1.
Lind, R. W. (1974). Shear-free, twisting Einstem-Maxwell metrics in the Newman-Penrose formalism, GRG 5, 25. See $$ 7.1., 23.1., 26.3.
Lind, R. W. (1975a). Gravitational and electromagnetic radiation in Kerr-Maxwett spaces, J. Math. Phys. 16, 34. See §§ 26.4., 26.5.
Lind, R. W. (1975b). Stationary Kerr-Maxwell spaces, J. Math. Phys. 16, 39. See $ 26.4.
Lindquist, R. W. See Boyer and Lindquist (1967)
Lorenc, P. See Horsky et al. (1977)
Lovelock, D. (1967). .4 spherically symmetric solution of.the Maxwett-Einslein equations, Commun. Math. Phys. 5, 257. See § 10.3.
Ludwig, G. (1969). Classificatiott of electromagnetic and gravitational fields, Amer. J. Pbys. 87, 1225. Seс $ 4.2.
390
Ludwig, G. (1970). Oeomelrodynamks of electromagnetic fields in the Xeu.-m«n Penro.se formalism, Commun. Math. Phys. 17, 98. See § 5.4.
Ludwig, G., and Scanlan, G. (1971). Clamijiealion of the Ricci tensor, Commun. Math. Pliys. 20, 291. See §5.1.
Lukiies, B. (1973). AU vacuum metrics with space-like symmetry and shearing geodesic timelike eigenrays, Report KFKI-1973-38, Centr. Res. Inst. Phys. Acad. Soi., Budapest. See § 16.5. Lukacs, B, (1974). AU stationary, rigidly rotating incoherent fluid metrics with geodesic IindllOr shear free eigenrays, Report KFKl-1974-87, Central Res. Inst. Phys. A< id. Sci.,-Budapest. See §§ 16.5,, 19.2.
Lukiies, B., and Perj?s, Z. (1973). Electrovac field* with geodesic, eigenrays, GRC 4.161. See § 1(1,5. Lukash, V. N. (1974). Gravitational waves Ihnt conserve the homogeneity of space (in Russian). Zh. Eksper. TeOr. Fiz. 67, 1594. See § 11.3.
Maartens, R., nnd Ne), S. D. (1978). Decomposable differential operators in « cosmological context, Commun, Math. Phys. 59, 273. See §§ 12.1.. 12.3., 12.4.
MaeCallum, М. A. H. (1971). .4 class of homogeneous cosmological models. I. Asymptotic behaviour, Commun. Math. Phys. 20, 57. See § 11.3.
MacCalIum, М. Л. H. (1972). On 'diagonal' Biunchi cosmologies, Phys. Letters A 40, 385. See §“-2-
MaeCallum, М. A. H. (1973). Cosmological models from a geometric point of view, in: Cargese Lectures in Physics, Vol. C, Gordon and Breach, Xew York. See § 11.2.
MacCaIlum, SI. A. H. (1979a). Anisotropic and inhomogeneous relativistic cosmologies, in: Hawking, .S. \V„ and Israel, W. (Ed.), General Belativitys an JEinstcin centenary survey. Cambridge Univ. Press. See § 11.2.
MaeCallum, М. A. H. (1979b). The mathematics of anisotropic cosmologies, in: Demianski, M. (Ed.), Proceedings of the First International Cracow Scbool of Cosmology, Springer-Verlag, Berlin, Heidelberg, New York. See § 11.2.
MaeCallum, М. A. H. (1979c). Oil the classification of ihe real fovr-dimcnsional Lie algebras. Preprint. See. § 8.2.
MaeCallum, М. A. H. (1980). Locally isotropic spacelimes Kith non-null homogeneous hyper-surfaces, in: Tipler1 F. J. (Ed.), Essays in General Relativity: a Festschrift for Abraham Taub, Academic Press. See § 11.1.
MaeCallum, М. A. H. See also EIIis nnd MaeCallum (1969)
МасСаІІшп, M. A. H., nnd Tnub, A. H. (1972). Variational principles and spatially homo-
geiuous universes including rotation. Commun. M-.ith. Phys. 25, 173. See § 11.2.
MaeCallum, M. A. H., Stewart, J. M., end Schmidt, B. G. (1970). Anisotropic stresses in homogeneous cosmologies, Commun. Math. Phys. 17, 343. See § 11.2.
Maison, D. (1978). Are the stationary, axially symmetric Einstein equations completely integrable?, Pliys. Rev. Lett. 41, 521. See §30.4.
Moitm, S. G. (1966). Stationary dust-filled co.-uioiogical solution with /1 = 0 and without closed timelike lines, J. Math. Phys. 7, 1025. See §§ 19.2., 20.2.
Majumd.ir, S. D. (1947). A doss of exact solutions of Einstein’s field equations, Phys. Rev. 72, 390. See §§ 16.7., 19.1.
Malhiot, R. J. See Hauser and MaIhiot (1974, 1975. 1976, 1978)
Marder, L. (1958a). Gravitational u'aves in general relativity. I, Cylindrical waves, Proc. Roy.
Soc. Lond. A 244, 524. See § 20.3.
Marder, L. (1958 b). Gravitational waves in general relativity. II. The reflexion of cylindrical waves, Proc. Roy. Soc. Lond. A 246. 133. See. § 20.3.