Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1895497 | Journal of Geometry and Physics | 2016 | 14 Pages |
Abstract
In Abdalla and Dillen (2002) an example of a non-semisymmetric Ricci-symmetric quasi-Einstein austere hypersurface M isometrically immersed in an Euclidean space was constructed. In this paper we state that, at every point of the hypersurface M, the following generalized Einstein metric curvature condition is satisfied: (â) the difference tensor Râ
CâCâ
R and the Tachibana tensor Q(S,C) are linearly dependent. Precisely, (nâ2)(Râ
CâCâ
R)=Q(S,C) on M. We also prove that non-conformally flat and non-Einstein hypersurfaces with vanishing scalar curvature having at every point two distinct principal curvatures, as well as some hypersurfaces having at every point three distinct principal curvatures, satisfy (â). We present examples of hypersurfaces satisfying (â).
Related Topics
Physical Sciences and Engineering
Mathematics
Mathematical Physics
Authors
Ryszard Deszcz, MaÅgorzata GÅogowska, Marian HotloÅ, Georges Zafindratafa,