Constrained \(f(Q, T)\) gravity accelerating cosmological model and its dynamical system analysis
DOI10.1016/j.nuclphysb.2023.116233zbMath1525.83031arXiv2305.08145MaRDI QIDQ6102073
M. Koussour, B. Mishra, Unnamed Author
Publication date: 20 June 2023
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.08145
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15) Constrained dynamics, Dirac's theory of constraints (70H45) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (1)
Cites Work
- Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
- FRW in quadratic form of \(f(T)\) gravitational theories
- Unification of constant-roll inflation and dark energy with logarithmic \(R^{{2}}\)-corrected and exponential \(F(R)\) gravity
- Energy conditions in modified gravity
- Relativistic Cosmology. I
- GEOMETRICAL DIAGNOSTIC FOR THE GENERALIZED CHAPLYGIN GAS MODEL
- Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity
- Cosmological perturbation theory in f(Q,T) gravity
- Flat FLRW Universe in logarithmic symmetric teleparallel gravity with observational constraints
- An alternative to quintessence
This page was built for publication: Constrained \(f(Q, T)\) gravity accelerating cosmological model and its dynamical system analysis
