“…In this regard, vacuum spatially homogeneous cosmologies, the Bianchi models, are expected to play a key role in the dynamical asymptotic behaviour, see [3,4,9,21,22]. Similarly, the Bianchi models derived in [10] are expected to describe generic singularities in Hořava gravity. In particular, it is heuristically argued that there is an 'asymptotically dominant' curvature term in (1.2d) toward the initial singularity, yielding a respective dominant Bianchi model.…”