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arxiv: 1009.2459 · v2 · pith:O3J6XHTRnew · submitted 2010-09-13 · 🌀 gr-qc · hep-th

f(T) modified teleparallel gravity models as an alternative for holographic and new agegraphic dark energy models

K. Karami , A. Abdolmaleki This is my paper
classification 🌀 gr-qc hep-th
keywords modelsgravityagegraphicholographicstatecorrespondingdarkenergy
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In the present work, we reconstruct different f(T)-gravity models corresponding to the original and entropy-corrected version 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 in 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.

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    In 5D f(T, T_G) gravity, thick branes develop splitting and internal structure controlled by the coupling, while supporting a normalizable chiral fermion zero mode and modified resonant Kaluza-Klein states due to the ...

  2. Quasinormal modes of the thick braneworld in $f(T)$ gravity

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