Toroidal solutions in 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.

12 pages, Latex. Version Published in IJMPA

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Cited by in corpus (7)

• The cosmological constant as an eigenvalue of the Hamiltonian constraint in Horava-Lifshits theory
• The Rotating Black Hole in Renormalizable Quantum Gravity: The Three-Dimensional Hořava Gravity Case
• Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
• Self-gravitational Interaction in z = 4 Horava-Lifshitz Gravity
• Spatially homogeneous black hole solutions in $z=4$ Hořava-Lifshitz gravity in $(4+1)$ dimensions with Nil geometry and $H^2\times R$ horizons
• The absence of the Kerr black hole in the Hořava-Lifshitz gravity
• Domain Wall solutions to Horava gravity