Anisotropic cosmology and (super)stiff matter in Hořava’s gravity theory
S. Kalyana RamaInstitute of Mathematical Sciences, C. I. T. Campus, Tharamani, Chennai 600 113, India
2009en
ABI
Аннотация
We study anisotropic cosmology in Ho\ifmmode \check{r}\else \v{r}\fi{}ava'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 $\ensuremath{\lambda}$. Also, Ho\ifmmode \check{r}\else \v{r}\fi{}ava's (super)renormalizable theory predicts (super)stiff matter whose equation of state is $p=w\ensuremath{\rho}$, with $w\ensuremath{\ge}1$. We discuss briefly the implications of these results for the nature of cosmological collapse.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
4 та иқтибос0 та фойдаланилган манба