$f(T)$ theories from holographic dark energy models

Abstract

We reconstruct $f(T)$ theories from three different holographic dark energy models in different time durations. For the HDE model, the dark energy dominated era with new setting up is chosen for reconstruction, and the radiation dominated era is chosen when the involved model changes into NADE. For the RDE model, radiation, matter and dark energy dominated time durations are all investigated. We also investigate the limitation which prevents an arbitrary choice of the time duration for reconstruction in HDE and NADE, and find that an improved boundary condition is needed for a more precise reconstruction of $f(T)$ theory.

arXiv comment15 pages

References in corpus (10)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• The World as a Hologram
• A Model of Holographic Dark Energy
• Einstein's Other Gravity and the Acceleration of the Universe
• Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
• Entropy Bounds and Dark Energy
• The final state and thermodynamics of dark energy universe
• A Dark Energy Model Characterized by the Age of the Universe
• Reconstructing Quintom from Ricci Dark Energy