Abstract
We consider the fractal Friedmann-Robertson-Walker universe filled with dark fluid. By making use of this assumption, we discuss two types of dark energy models: Generalized Ricci and generalized holographic dark energies. We calculate the equation-of-state parameters, investigate some special limits of the results and discuss the physical implications via graphs. Also, we reconstruct the potential and the dynamics of the quintessence and k-essence (kinetic-quintessence) according to the results obtained for the fractal dark energy.
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Salti, M., Korunur, M. & Acikgoz, I. Extended Ricci and holographic dark energy models in fractal cosmology. Eur. Phys. J. Plus 129, 95 (2014). https://doi.org/10.1140/epjp/i2014-14095-1
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DOI: https://doi.org/10.1140/epjp/i2014-14095-1