Salti, M.Korunur, M.Acikgoz, I.2024-04-242024-04-2420142190-5444https://doi.org/10.1140/epjp/i2014-14095-1https://hdl.handle.net/11468/17819We 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.eninfo:eu-repo/semantics/closedAccess[No Keyword]Article1295WOS:0003372726000012-s2.0-8492257592310.1140/epjp/i2014-14095-1Q1Q2