arXiv · hep-th/0510183
Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity
Abstract
The solution of dark energy problem in the models without scalars is presented. It is shown that late-time accelerating cosmology may be generated by the ideal fluid with some implicit equation of state. The universe evolution within modified Gauss-Bonnet gravity is considered. It is demonstrated that such gravitational approach may predict the (quintessential, cosmological constant or transient phantom) acceleration of the late-time universe with natural transiton from deceleration to acceleration (or from non-phantom to phantom era in the last case).
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Shin'ichi Nojiri, Sergei D. Odintsov, O. G. Gorbunova. 2005-11-22. Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity. https://doi.org/10.1088/0305-4470%2F39%2F21%2Fs62
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