Late time acceleration in Brans Dicke Cosmology
arXiv:gr-qc/0010092 · doi:10.1103/PhysRevD.63.124006
Abstract
In this work we have investigated the possibility of having a late time accelerated phase of the universe, suggested by recent supernova observation, in the context of Brans Dicke (BD) theory with a symmetry breaking potential and a matter field. We find that a perfect fluid matter field (pressureless and with pressure) cannot support this acceleration but a fluid with dissipative pressure can drive this late time acceleration. We have also calculated some cosmological parameters in our model to match with observations.
8 pages, RevTex style, 3 postscript figures, some more Comments made about the feature of the model, references included, typos corrected. Accepted for publication in Phys.Rev.D
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