  We study Euclidean wormholes in the framework of the Horava-Lifshitz theory
of gravity. Euclidean wormholes first appeared in the Euclidean path integral
approach to quantum gravity. In a more general way, Hawking and Page
interpreted such configurations as solutions to the Wheeler-DeWitt equation
with appropriate boundary conditions. We use the projectable version of
Horava-Lifshitz gravity to obtain the Wheeler-DeWitt equation of a
minisuperspace model considering a closed Friedmann Universe plus a massless
scalar field. For large values of the scale factor we find that the solution of
the Wheeler-DeWitt equation coincides with the one obtained by Hawking. Whereas
in the limit corresponding to the early Universe we find a new set of
solutions, which agree with the Hawking and Page boundary conditions for
wormholes.
