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We study anisotropic cosmology in Ho r rava'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. Also, Ho r rava's (super) renormalizable theory predicts (super) stiff matter whose equation of state is p=w, with w1. We discuss briefly the implications of these results for the nature of cosmological collapse.
S. Kalyana Rama (Fri,) studied this question.
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