Extremal rotating solutions in Hořava gravity
Ahmad GhodsiDepartment of Physics, Ferdowsi University of Mashhad, P.O. Box 1436, Mashhad, IranEhsan HatefiDepartment of Physics, Ferdowsi University of Mashhad, P.O. Box 1436, Mashhad, Iran
2010en
ABI
Abstract
Recently a new four-dimensional nonrelativistic renormalizable theory of gravity was proposed by Ho\ifmmode \check{r}\else \v{r}\fi{}ava. In this paper we have found different near horizon geometries in Ho\ifmmode \check{r}\else \v{r}\fi{}ava gravity. We find the rotating solutions in a special range of parameters of the theory. This range allows us to include up to six derivative terms in the equations of motion. We have found our solutions as perturbed solutions over spherical symmetric background with small rotating parameter.
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