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On spacelike hypersurfaces of constant sectional curvature lorentz manifolds
Institution:1. Centro de Análise Matemática, Geometria e Sistemas Dinâmicos, Instituto Superior Técnico, Lisboa, Portugal;2. Department of Mathematical Sciences, Chalmers University of Technology, University of Gothenburg, Gothenburg, Sweden;3. Departamento de Matemática e Aplicações, Universidade do Minho, Guimarães, Portugal;4. Centro de Matemática, Universidade do Minho, Braga, Portugal;1. Fenomenos Nonlineales y Mecánica (FENOMEC), Department of Mathematics and Mechanics, Instituto de Investigacion en Matemáticas Aplicadas y Sistemas, Universidad Nacional Autónoma de México, 01000 México D.F., Mexico;2. School of Mathematics and Applied Statistics, University of Wollongong, Northfields Avenue, Wollongong, New South Wales, 2522, Australia;3. School of Mathematics and Maxwell Institute for Mathematical Sciences, University of Edinburgh, Edinburgh EH9 3FD, Scotland, UK
Abstract:Let x:MnM¯n+1 be an n-dimensional spacelike hypersurface of a constant sectional curvature Lorentz manifold M¯. Based on previous work of S. Montiel, L. Alías, A. Brasil and G. Colares studied what can be said about the geometry of M when M¯ is a conformally stationary spacetime, with timelike conformal vector field K. For example, if Mn has constant higher order mean curvatures Hr and Hr+1, they concluded that Mn is totally umbilical, provided Hr+10 on it. If div(K) does not vanish on Mn they also proved that Mn is totally umbilical, provided it has, a priori, just one constant higher order mean curvature.In this paper, we compute Lr(Sr) for such an immersion, and use the resulting formula to study both r-maximal spacelike hypersurfaces of M¯, as well as, in the presence of a constant higher order mean curvature, constraints on the sectional curvature of M that also suffice to guarantee the umbilicity of M. Here, by Lr we mean the linearization of the second order differential operator associated to the r-th elementary symmetric function Sr on the eigenvalues of the second fundamental form of x.
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