Smooth cosmological phase transition in the Horava-Lifshitz gravity

Understand

We show that the cosmological phase transition from the first accelerated expansion in the early universe to the second accelerated expansion over the intermediate decelerated expansion is possible in the HL gravity without the ``detailed balance'' condition if the dark scalar energy density is assumed to be negative.

• Moreover, we obtain various evolutions depending on the scale factor and the expansion rate.
• Finally, we discuss the existence of the minimum scale in connection with the singularity free condition.