Generalised scalar-tensor theory and the cosmic acceleration
| Autor: | Banerjee, Narayan, Ganguly, Koyel |
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| Rok vydání: | 2008 |
| Předmět: | |
| Zdroj: | Int.J.Mod.Phys.D18:445-451,2009 |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1142/S0218271809014479 |
| Popis: | In this paper it has been shown that a simple functional form of $\omega(\phi)$ in a generalised scalar tensor theory can drive the present cosmic acceleration without any quintessence field or the cosmological constant $\Lambda$. Furthermore, it ensures a smooth transition from a decelerated to an accelerated phase of expansion in the matter dominated regime. Comment: Typos (author's name!)corrected |
| Databáze: | arXiv |
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