Abstract
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.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
