“…Further we notice that for holomorphically projective mappings between e-Kähler manifolds K n andK n of class C 3 holds the following third set of equations [6,8,9,15,10,16]:…”
Section: On Holomorphically Projective Mappings Of E-kähler Manifoldsmentioning
confidence: 99%
“…We present well known facts, which were proved by Domashev, Kurbatova, Mikeš, Prvanović, Otsuki, Tashiro etc., see [2,3,6,7,8,9,10,11,12,15,16,17,18,19]. In these results no details about the smoothness class of the metric were stressed.…”
“…Further we notice that for holomorphically projective mappings between e-Kähler manifolds K n andK n of class C 3 holds the following third set of equations [6,8,9,15,10,16]:…”
Section: On Holomorphically Projective Mappings Of E-kähler Manifoldsmentioning
confidence: 99%
“…We present well known facts, which were proved by Domashev, Kurbatova, Mikeš, Prvanović, Otsuki, Tashiro etc., see [2,3,6,7,8,9,10,11,12,15,16,17,18,19]. In these results no details about the smoothness class of the metric were stressed.…”
“…From that follows F 2 = κ Id, where κ is a function, which is in contradiction with our assumption. For this reason in the formula (22) we suppose that…”
Section: On F ε 2 -Planar Mappings Of (Pseudo-) Riemannian Manifolds 291mentioning
“…In 1978 (see [15] and PhD. thesis [14], and see [16,21,22], [23, p. 125], [25, p. 188]) Mikeš proved that under the conditions V n ,V n ∈ C 3 the following theorem holds (locally):…”
Section: Geodesic Mappings Of Einstein Manifoldsmentioning
confidence: 99%
“…We briefly remind some main facts of geodesic mapping theory of (pseudo-) Riemannian manifolds which were found by T. Levi-Civita [13], L.P. Eisenhart [5,6] and N.S. Sinyukov [31], see [1,[9][10][11]14,16,18,19,23,[25][26][27][28][29][30][31][32][34][35][36]. In these results no details about the smoothness class of the metric were stressed.…”
In this paper we prove that geodesic mappings of (pseudo-) Riemannian manifolds preserve the class of differentiability (C r , r ≥ 1). Also, if the Einstein space Vn admits a non trivial geodesic mapping onto a (pseudo-) Riemannian manifoldVn ∈ C 1 , thenVn is an Einstein space. If a four-dimensional Einstein space with non constant curvature globally admits a geodesic mapping onto a (pseudo-) Riemannian manifoldV4 ∈ C 1 , then the mapping is affine and, moreover, if the scalar curvature is non vanishing, then the mapping is homothetic, i.e.ḡ = const · g.1991 Mathematics Subject Classification. 53B20, 53B21, 53B30, 53C25.
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