  The recently proposed Horava-Lifshitz (HL) theory of gravity is analyzed from
the quantum cosmology point of view. By employing usual quantum cosmology
techniques, we study the quantum Friedmann-Lemaitre-Robertson-Walker (FLRW)
universe filled with radiation in the context of HL gravity. We find that this
universe is quantum mechanically nonsingular in two different ways: the
expectation value of the scale factor $<a>(t)$ never vanishes and, if we
abandon the detailed balance condition suggested by Horava, the quantum
dynamics of the universe is uniquely determined by the initial wave packet and
no boundary condition at $a=0$ is indeed necessary.
