Logamediate Inflation in f(T) Teleparallel Gravity
arXiv:1702.07877 · doi:10.3847/1538-4357/aa5c83
Abstract
We study logamediate inflation in the context of teleparallel gravity. -gravity is a generalization of the teleparallel gravity which is formulated on the Weitzenböck spacetime, characterized by the vanishing curvature tensor (absolute parallelism) and the non-vanishing torsion tensor. We consider an -gravity model which is sourced by a canonical scalar field. Assuming a power-law function in the action, we investigate an inflationary universe with a logamediate scale factor. Our results show that, although logamediate inflation is completely ruled out by observational data in the standard inflationary scenario based on Einstein gravity, it can be compatible with the 68\% confidence limit joint region of Planck 2015 TT,TE,EE+lowP data in the framework of -gravity.
12 pages, 2 figures
References in corpus (20)
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- On Born-Infeld Gravity in Weitzenbock spacetime
- Cosmological perturbations in f(T) gravity
- Observational constraints on theory
- f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
- models with phantom divide line crossing
- Degrees of freedom of gravity
- Growth factor in f(T) gravity
- Observational information for f(T) theories and Dark Torsion
- Conformal transformation in theories
- Linking Tests of Gravity On All Scales: from the Strong-Field Regime to Cosmology
- Inflationary universe from perfect fluid and gravity and its comparison with observational data
- Dynamics of Logamediate Inflation
- Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
- Translation of Einstein's Attempt of a Unified Field Theory with Teleparallelism
- A class of quintessential inflation models with parameter space consistent with BICEP2
- Inflation and dark energy from f(R) gravity
- Inflation with teleparallelism: Can torsion generate primordial fluctuations without local Lorentz symmetry?