Cosmic evolution in f(T) gravity theory

Abstract

The paper deals with cosmology in modified f(T) gravity theory. With some phenomenological choices for the function f(T) it is possible to have cosmological solutions describing different phases of the evolution of the Universe for the homogeneous and isotropic FLRW model. By proper choice of the parameters involved in the function $f(T)$ and also in the cosmological solutions it is shown that a continuous cosmic evolution starting from the emergent scenario to the present late time acceleration is possible. Finally thermodynamical analysis of f(T) gravity is presented.

References in corpus (15)

• Dark torsion as the cosmic speed-up
• Einstein's Other Gravity and the Acceleration of the Universe
• Cosmological perturbations in f(T) gravity
• Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields
• Growth factor in f(T) gravity
• Nonminimal torsion-matter coupling extension of f(T) gravity
• Static Solutions with Spherical Symmetry in f(T) Theories
• Generalized Second Law of Thermodynamics in $f(T)$ Gravity with Entropy Corrections
• Is Emergent Universe a Consequence of Particle Creation Process?
• Resolution of dark matter problem in f(T) gravity
• Interacting Dark Energy in f(T) cosmology : A Dynamical System analysis
• A type of Born-Infeld regular gravity and its cosmological consequences
• Phenomenological Reconstruction of $f(T)$ Teleparallel Gravity
• Reconstructions of $f(T)$ Gravity from Entropy Corrected Holographic and New Agegraphic Dark Energy Models in Power-law and Logarithmic Versions
• An Emergent Universe supported by chiral cosmological fields in Einstein--Gauss--Bonnet gravity