Wormholes in Horava gravity with cosmological constant

摘要: By combining analytical and numerical methods we find that the solutions of complete Horava theory with negative cosmological constant satisfy conditions staticity, spherical symmetry vanishing shift function are two kinds geometry: (i) a wormhole-like solution sides joined by throat (ii) single side naked singularity at origin. We study second-order effective action. consider case when coupling (partial ln N)^2 term, which is unique deviation from general relativity in action, small. At one wormhole acquires kind deformed AdS asymptotia other there an asymptotic essential singularity. The deformation essentially means lapse N diverges asymptotically bit faster than AdS. This can also be interpreted as anisotropic Lifshitz scaling acquire asymptotically.