To theory of asymptotically stable accelerating Universe in Riemann-Cartan spacetime
arXiv:1410.0460 · doi:10.1088/1475-7516/2014/12/027
Abstract
Homogeneous isotropic cosmological models built in the framework of the Poincaré gauge theory of gravity based on general expression of gravitational Lagrangian with indefinite parameters are analyzed. Special points of cosmological solutions for flat cosmological models at asymptotics and conditions of their stability in dependence of indefinite parameters are found. Procedure of numerical integration of the system of gravitational equations at asymptotics is considered. Numerical solution for accelerating Universe without dark energy is obtained.
arXiv comment13 pages, 3 figures. arXiv admin note: substantial text overlap with arXiv:1107.1566
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Cited by in corpus (4)
- Cosmology in Poincare gauge gravity with a pseudoscalar torsion
- Self-accelerating Universe in modified gravity with dynamical torsion
- On the stability of self-accelerating Universe in modified gravity with dynamical torsion
- Gauge gravitation theory in Riemann-Cartan space-time and gravitational interaction