  We perform a detailed phase-space analysis of Horava-Lifshitz cosmology, with
and without the detailed-balance condition. Under detailed-balance we find that
the universe can reach a bouncing-oscillatory state at late times, in which
dark-energy, behaving as a simple cosmological constant, is dominant. In the
case where the detailed-balance condition is relaxed, we find that the universe
reaches an eternally expanding, dark-energy-dominated solution, with the
oscillatory state preserving also a small probability. Although this analysis
indicates that Horava-Lifshitz cosmology can be compatible with observations,
it does not enlighten the discussion about its possible conceptual and
theoretical problems.

High Energy Physics - Theory;Cosmology and Nongalactic Astrophysics;General Relativity and Quantum Cosmology