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We study Euclidean wormholes in the framework of the Horava-Lifshitz theoryof gravity. Euclidean wormholes first appeared in the Euclidean path integralapproach to quantum gravity. In a more general way, Hawking and Pageinterpreted such configurations as solutions to the Wheeler-DeWitt equationwith appropriate boundary conditions. We use the projectable version ofHorava-Lifshitz gravity to obtain the Wheeler-DeWitt equation of aminisuperspace model considering a closed Friedmann Universe plus a masslessscalar field. For large values of the scale factor we find that the solution ofthe Wheeler-DeWitt equation coincides with the one obtained by Hawking. Whereasin the limit corresponding to the early Universe we find a new set ofsolutions, which agree with the Hawking and Page boundary conditions forwormholes.

Euclidean Wormholes in Horava-Lifshitz Gravity