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- W3100691691 abstract "Evolution of a background space-time metric and sub-horizon matter density perturbations in the Universe is numerically analyzed in viable $f(R)$ models of present dark energy and cosmic acceleration. It is found that viable models generically exhibit recent crossing of the phantom boundary $w_{rm DE}=-1$. Furthermore, it is shown that, as a consequence of the anomalous growth of density perturbations during the end of the matter-dominated stage, their growth index evolves non-monotonically with time and may even become negative temporarily." @default.
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- W3100691691 date "2010-05-01" @default.
- W3100691691 modified "2023-10-17" @default.
- W3100691691 title "Phantom Boundary Crossing and Anomalous Growth Index of Fluctuations in Viable f(R) Models of Cosmic Acceleration" @default.
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- W3100691691 doi "https://doi.org/10.1143/ptp.123.887" @default.
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