https://doi.org/10.1140/epjp/i2015-15164-7
Regular Article
Behaviour of f(T) dark energy model in fractal cosmology
1
Physics department, Faculty of science, Damnhour University, Damnhour, Egypt
2
Theoretical Research Group, Physics department, Faculty of science, Dameitta University, 34517, New Damietta City, Egypt
* e-mail: ayman.aly@cern.ch
Received:
7
April
2015
Revised:
13
July
2015
Accepted:
27
July
2015
Published online:
20
August
2015
The f(T) modified gravity model is considered in the framework of fractal space-time. Assuming only the time has a fractal profile while the other spatial coordinates have their normal geometrical descriptions, the Hubble parameter, H, the dark energy density, 
, the deceleration parameter, q, the pressure P, and state finder parameters r and s are reconstructed for our model. It is interesting to mention here that all the results are consistent with the recent present observations.
© Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg, 2015
