Speaker
Mrs
Asrin Abdolmaleki
(Department of Physics, University of Kurdistan)
Description
In the present work, we reconstruct the different f(T)-gravity
models corresponding to the original and entropy-corrected versions
of the holographic and new agegraphic dark energy models. We also
obtain the equation of state parameters of the corresponding
f(T)-gravity models. We conclude that the holographic and new
agegraphic f(T)-gravity models behave like phantom or quintessence
model. Whereas for the entropy-corrected models, the equation of
state parameter can justify the transition from the quintessence
state to the phantom regime as indicated by the recent observations.
Primary author
Mrs
Asrin Abdolmaleki
(Department of Physics, University of Kurdistan)
Co-author
Prof.
Kayoomars Karami
((1) Department of Physics, University of Kurdistan, Pasdaran St., Sanandaj, Iran (2) Research Institute for Astronomy and Astrophysics of Maragha (RIAAM), Maragha, Iran)
