LCDM Model in f(T) Gravity: Reconstruction, Thermodynamics and Stability
arXiv:1307.0730 · doi:10.1088/1475-7516/2013/11/060
Abstract
We investigate some cosmological features of the LCDM model in the framework of the generalized teleparallel theory of gravity f(T) where T denotes the torsion scalar. Its reconstruction is performed giving rise to an integration constant Q and other input parameters according to which we point out more analysis. Thereby, we show that for some values of this constant, the first and second laws of thermodynamics can be realized in the equilibrium description, for the universe with the temperature inside the horizon equal to that at the apparent horizon. Moreover, still within these suitable values of the constant, we show that the model may be stable using the de Sitter and Power-Law cosmological solutions.
25 pages, 2 figures, Accepted for publication in Journal of Cosmology and Astroparticle Physics (JCAP)
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- Stability of the flat FLRW metric in gravity
- Junction conditions in extended Teleparallel gravities
- Generalized teleparallel cosmology and initial singularity crossing
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- Distinguish the model from CDM model with Gravitational Wave observations
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