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

Abstract

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.

22 pages, 8 figures, the preprint has been improved considerably

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• Constraining the Schwarzschild-de Sitter Solution in Models of Modified Gravity
• Born-Infeld and Charged Black Holes with non-linear source in $f(T)$ Gravity
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• Spherical Accretion of Matter by Charged Black Holes on f(T) Gravity
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• Evaporation phenomena in f(T) gravity
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• Power Law Entropy Corrected New-Agegraphic Dark Energy in Hořava-Lifshitz Cosmology
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• Starobinsky Inflation and Dark Energy and Dark Matter Effects from Quasicrystal Like Spacetime Structures
• Polytropic Stars in $f(Q)=Q+\xi Q^2$ covariant formulation
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