Hypersurfaces in space forms satisfying some curvature conditions
详细信息    查看全文
文摘
In Abdalla and Dillen (2002) an example of a non-semisymmetric Ricci-symmetric quasi-Einstein austere hypersurface dd1a4577c8554ebda3f855c797fd3c4e" title="Click to view the MathML source">M isometrically immersed in an Euclidean space was constructed. In this paper we state that, at every point of the hypersurface dd1a4577c8554ebda3f855c797fd3c4e" title="Click to view the MathML source">M, the following generalized Einstein metric curvature condition is satisfied: () the difference tensor cdd6da4c6cc221e3302abdc9e0149" title="Click to view the MathML source">R⋅C−C⋅R and the Tachibana tensor Q(S,C) are linearly dependent. Precisely, View the MathML source on dd1a4577c8554ebda3f855c797fd3c4e" title="Click to view the MathML source">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 (). We present examples of hypersurfaces satisfying ().

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700