Investigating the compatibility of exact solutions in Weyl-type \(f(Q, T)\) gravity with observational data

DOI10.1142/S0219887824400139zbMATH Open1547.83127MaRDI QIDQ6601416

M. Koussour, S. Myrzakulova, Nurgissa Myrzakulov

Publication date: 10 September 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

Hubble parameteraccelerated expansiondark energynon-metricity\(f(Q, T)\) gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)

Cites Work

• Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off
• Model-independent reconstruction of \(f(Q)\) non-metric gravity
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• New general relativity
• The cosmological constant and dark energy
• Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity
• Cosmological perturbation theory in f(Q,T) gravity
• Modified gravity as an alternative for ΛCDM cosmology
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• A New Parametrization of Hubble Parameter in f(Q)$f(Q)$ Gravity
• Anisotropic universe in \(f(Q,T)\) gravity, a novel study
• Constrained \(f(Q, T)\) gravity accelerating cosmological model and its dynamical system analysis
• On a Bianchi type-I space-time with bulk viscosity in f(R,T) gravity
• A model-independent method with phantom divide line crossing in Weyl-type \(f(Q, T)\) gravity

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