TL;DR
This paper explores toroidal solutions in Horava gravity, a non-relativistic renormalizable theory, focusing on near horizon geometries with slow rotation, extending understanding of its solution space.
Contribution
It introduces new toroidal solutions within Horava gravity using a novel action, highlighting near horizon geometries with slow rotation.
Findings
Derived explicit toroidal solutions in Horava gravity.
Described near horizon geometries with slow rotation.
Extended the solution space of Horava gravity.
Abstract
Recently a new four-dimensional non relativistic renormalizable theory of gravity was proposed by Horava. This gravity reduces to Einstein gravity at large distances. In this paper by using the new action for gravity we present different toroidal solutions to the equations of motion. Our solutions describe the near horizon geometry with slow rotating parameter.
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