2015/10/18 by G. G. L. Nashed, Nashed, G. G. L., W. El Hanafy +1
Earth and Planetary Sciences · Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #General Physics (physics.gen-ph) #General Relativity and Quantum Cosmology (gr-qc) #Geophysics and Gravity Measurements #Relativity and Gravitational Theory #gr-qc #physics.gen-ph
paper · pdf · doi:10.48550/arxiv.1511.01445
This paper has been withdrawn by the authors due to the due to the inconvenient classification of the arXiv
openalex publication_date 2015/10/18 · arxiv created 2015/11/05 · arxiv updated 2015/11/06 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
A cubic correction of f(T) gravity, where T is the teleparallel scalar torsion, is considered to describe gravity in spatially flat Friedmann-Robertson-Walker model. A scale factor permitting departure from inflation era has been derived. The cosmological evolution has been studied and it has shown that a phase transition from early era to late one is possible. The maximum temperature by releasing the vacuum latent heat has been shown to be much below the GUT temperature. The energy conditions have been analyzed and has shown that they are satisfied for certain values of the parameters ε and β. The cosmographic parameters are used and has been shown that the derived solution satisfies f(T) and its higher derivatives up to fourth order.