Jhingan, S. ; Nojiri, S. ; Odintsov, S. D. ; Sami, M. ; Thongkool, I. ; Zerbini, S. (2008) Phantom and non-phantom dark energy: the cosmological relevance of non-locally corrected gravity Physics Letters B, 663 (5). pp. 424-428. ISSN 0370-2693
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Official URL: http://www.sciencedirect.com/science/article/pii/S...
Related URL: http://dx.doi.org/10.1016/j.physletb.2008.04.054
Abstract
In this letter we have investigated the cosmological dynamics of non-locally corrected gravity involving a function of the inverse d'Alembertian of the Ricci scalar, f(□-1R). Casting the dynamical equations into local form, we derive the fixed points of the dynamics and demonstrate the existence and stability of a one parameter family of dark energy solutions for a simple choice,f(□−1R)˜exp(α□−1R). The effective EoS parameter is given by, weff=(α−1)/(3(α−1) and the stability of the solutions is guaranteed provided that 1/3<α<2/3. For 1/3<α<1/2 and 1/2<α<2/3, the underlying system exhibits phantom and non-phantom behavior respectively; the de Sitter solution corresponds to α=1/2. For a wide range of initial conditions, the system mimics dust like behavior before reaching the stable fixed point. The late time phantom phase is achieved without involving negative kinetic energy fields. A brief discussion on the entropy of de Sitter space in non-local model is included.
Item Type: | Article |
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Source: | Copyright of this article belongs to Elsevier Science. |
ID Code: | 70508 |
Deposited On: | 21 Nov 2011 05:42 |
Last Modified: | 21 Nov 2011 05:42 |
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