Anisotropic cosmology and (super)stiff matter in Horava's gravity theory

We study anisotropic cosmology in Horava's gravity theory and obtain Kasner-type solutions, valid for any number, d, of spatial dimensions. The corresponding exponents satisfy two relations, one involving the marginal coupling lambda. Also, Horava's (super)renormalizable theory predicts ( super) stiff matter whose equation of state is p = w rho, with w >= 1. We discuss briefly the implications of these results for the nature of cosmological collapse.