2004/06/03 by Fernando Dobarro, Bulent Unal · 2 citations
Mathematics · Physics and Astronomy · #math.FA #gr-qc #math.AP #math.DG #msc:53C25 #msc:53C50 #msc:53C80
published as Nonlinear Anal. 59 (2004) 759-770 · 16 pages, submitted to Nonlinear Analysis TMA
arxiv created 2004/06/03 · arxiv updated 2009/12/01
Essentially, some conditions for the Riemannian factor and the warping function of a standard static space-time are obtained in order to guarantee that no nontrivial warping function on the Riemannian factor can make the standard static space-time Einstein.