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

K. Karami , A. Abdolmaleki

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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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Quasinormal modes of the thick braneworld in $f(T)$ gravity
gr-qc 2026-04 unverdicted novelty 5.0

In a thick braneworld model with f(T) = T + α T², the parameter α induces brane splitting and alters the decay rates of quasinormal modes, with two numerical methods agreeing on the low-overtone spectrum.