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We have considered the modified and the extended holographic Riccidark energy models (MHRDE and EHRDE) in fractal universe. We have assumed a time-likefractal profile   v  =   t   −  β    , where   β  =  4   (   1  −  α   )   . We have reconstructed the Hubble parameter   H   , the energy density, the equations of state parameter    w,    and the deceleration parameter    q    for both MHRDE and EHRDE.

A Study on Some Special Forms of Holographic Ricci Dark Energy in Fractal Universe