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We obtain the static spherically symmetric vacuum solutions ofHorava-Lifshitz gravity theory, imposing the detailed balance condition only inthe UV limit. We find the solutions in two different coordinate systems, thePainlev\'e-Gullstrand coordinates and the Poincare coordinates, to examine theconsequences of imposing the projectability condition. The solutions in twocoordinate systems are distinct due to the non-relativistic nature of the HLgravity. In the Painleve-Gullstrand coordinates complying with theprojectability condition, the solution involves an additional integrationconstant which yields surplus angle and implies attractive Coulomb forcebetween same charges.

Surplus Angle and Sign-flipped Coulomb Force in Projectable Horava-Lifshitz Gravity