Onset of acceleration in a Universe initially filled by dark and baryonic matters in nonminimally coupled teleparallel model
arXiv:1510.02085 · doi:10.1103/PhysRevD.92.123538
Abstract
A nonminimally coupled quintessence dark energy in teleparallel model of gravity is considered. It is clarified how a matter dominated universe with initial negligible dark energy density can evolve to a late time de Sitter space-time via the symmetry breaking.
16 pages, 3 figures, accepted for publication in Physical Review D
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Cited by in corpus (18)
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- Covariant formulation of scalar-torsion gravity
- New observational constraints on f(T) gravity from cosmic chronometers
- Dynamical system analysis for nonminimal torsion-matter coupled gravity
- Mass varying neutrinos, symmetry breaking, and cosmic acceleration
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- Inflation with teleparallelism: Can torsion generate primordial fluctuations without local Lorentz symmetry?
- Reheating in a modified teleparallel model of inflation
- Cosmic acceleration and de Sitter expansion in hybrid mass varying neutrino model
- Dynamics of a higher-dimension Einstein-Scalar-Gauss-Bonnet cosmology
- Symmetry breaking, and the effect of matter density on neutrino oscillation
- Cosmic acceleration in screening hybrid quintessence model
- Late-time power-law stages of cosmological evolution in teleparallel gravity with nonminimal coupling
- Avoiding parameter fine-tuning in mass varying neutrino models of DE?
- Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
- Imprints of vector field non-standard couplings on solar neutrino flux
- Global portraits of nonminimal teleparallel inflation