Cosmological Evolution for Dark Energy Models in f(T) Gravity

Abstract

In this paper, we investigate the behavior of equation of state parameter and energy density for dark energy in the framework of f(T) gravity. For this purpose, we use anisotropic LRS Bianchi type I universe model. The behavior of accelerating universe is discussed for some well-known f(T) models. It is found that the universe takes a transition between phantom and non-phantom phases for f(T) models except exponential and logarithmic models. We conclude that our results are relativity analogous to the results of FRW universe.

22 pages, 16 figures, some references are added

References in corpus (15)

• Dark torsion as the cosmic speed-up
• Modified teleparallel gravity: inflation without inflaton
• Einstein's Other Gravity and the Acceleration of the Universe
• Two new diagnostics of dark energy
• $f(T)$ models with phantom divide line crossing
• Conformal transformation in $f(T)$ theories
• Cosmological evolution in exponential gravity
• Dynamics of Bianchi I Universe with Magnetized Anisotropic Dark Energy
• Gravitational Perfect Fluid Collapse in f(R) Gravity
• Effects of Electromagnetic Field on the Dynamics of Bianchi type $V{I}_0$ Universe with Anisotropic Dark Energy
• Non-vacuum Solutions of Bianchi Type VI_0 Universe in f(R) Gravity
• Cosmological constraints on the Hu-Sawicki modified gravity scenario
• Effects of f(R) Dark Energy on Dissipative Anisotropic Collapsing Fluid
• L.R.S. Bianchi type II Stiff Fluid cosmological model with Decaying Vacuum Energy Density $\Lambda$ in general relativity
• Energy Contents of Some Well-Known Solutions in Teleparallel Gravity

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• Warm Intermediate Inflation in $F(T)$ Gravity
• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• Models of Collapsing and Expanding Anisotropic Gravitating Source in $f(R,T)$ Theory of Gravity
• Renormalizability of alternative theories of gravity: differences between power counting and entropy argument
• Transient acceleration in $f(T)$ gravity
• Static plane symmetric solutions in $f(Q)$ gravity