Abstract
We present some solutions showing evolution from early inflation to late time acceleration in FLRW space time with Gauss-Bonnet term and ideal fluid. In the late time era, we have either quintessence, or phantom or de-Sitter era of expansion depending on the parameters. The Chameleon mechanism shows that the correction to the Newton’s law could be small.
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B. Modak acknowledges PURSE, DST(India) for financial support.
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Dutta, M.K., Modak, B. Late Time Acceleration and Chameleon Cosmology in Gauss Bonnet Theory. Int J Theor Phys 54, 2591–2604 (2015). https://doi.org/10.1007/s10773-014-2490-1
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DOI: https://doi.org/10.1007/s10773-014-2490-1