2004
DOI: 10.1016/s0362-546x(04)00286-x
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Special standard static space–times

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.

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Cited by 5 publications
(6 citation statements)
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“…Analogously, in several articles the following problem has been studied (see [12,26,36,37,38,42,43,44,74,108] among others).…”
Section: Introductionmentioning
confidence: 99%
“…Analogously, in several articles the following problem has been studied (see [12,26,36,37,38,42,43,44,74,108] among others).…”
Section: Introductionmentioning
confidence: 99%
“…In Lorentzian geometry, it was first noticed that some well known solutions to Einstein's field equations can be expressed in terms of warped products in [12] and after that Lorentzian warped products have been used to obtain more solutions to Einstein's field equations (see [12,13,19,20,44,59,65]). Moreover, geometric properties such as geodesic structure or curvature of Lorentzian warped products have been studied by many authors because of their relativistic applications (see [2,3,4,5,10,11,14,17,22,23,28,30,32,33,34,36,37,45,50,55,56,63,67,68,69,70,71,74,75]). …”
Section: Introductionmentioning
confidence: 99%
“…Moreover, in [56], the conformal tensor on standard static space-times with perfect fluid is studied and it is shown that a standard static space-time with perfect fluid is conformally flat if and only if its fiber is Einstein and hence of constant curvature. In [28], this problem is considered for arbitrary standard static space-times, more explicitly, an essential investigation of conditions for the fiber and warping function for a standard static space-time (not necessarily with perfect fluid) is carried out so that there exists no nontrivial function on the fiber guaranteing that the standard static space-time is Einstein. Duggal studied the scalar curvature of 4-dimensional triple Lorentzian products of the form L × B × f F and obtained explicit solutions for the warping function f to have a constant scalar curvature for this class of products (see [30]).…”
Section: Introductionmentioning
confidence: 99%
“…Generalized Robertson-Walker space-times and standard static space-times are two well known solutions to Einstein's field equations. The standard static space-times can be considered as a generalization of the Einstein static universe [12]. In addition, the Robertson-Walker models in general relativity describe a simply connected homogeneous isotropic expanding or contracting universe.…”
Section: Applicationsmentioning
confidence: 99%