Cosmological implications of the constant jerk parameter in \(f(Q, T)\) gravity theory

DOI10.1016/j.cjph.2023.10.001zbMATH Open1540.83102MaRDI QIDQ6543461

Nurgissa Myrzakulov, Alnadhief H. A. Alfedeel, M. Koussour, H. M. Elkhair

Publication date: 24 May 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

zbMATH Keywords

dark energynon-metricityjerk parameter\(f(Q, T)\) gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Dark matter and dark energy (83C56)

Cites Work

• A dark energy model characterized by the age of the Universe
• Quantum de Sitter cosmology and phantom matter
• A new type of isotropic cosmological models without singularity
• In search of the dark matter dark energy interaction: a kinematic approach
• Jerk, snap and the cosmological equation of state
• Cosmological perturbation theory in f(Q,T) gravity
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Reconstruction of cosmic history from a simple parametrization of H
• The cosmological constant problem
• An alternative to quintessence
• A New Parametrization of Hubble Parameter in f(Q)$f(Q)$ Gravity
• Transit cosmological models in modified f(Q,T) gravity
• FRW cosmology in f(Q,T) gravity
• Symmetric teleparallel general relativity

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