Statistical and observation comparison of Weyl-type \(f(Q, T)\) models with the \(\Lambda\)CDM paradigm

DOI10.1016/j.nuclphysb.2024.116727MaRDI QIDQ6653833

A. Bouali, Himanshu Chaudhary, P. K. Sahoo, Gaurav N. Gadbail

Publication date: 17 December 2024

Published in: Nuclear Physics B (Search for Journal in Brave)

zbMATH Keywords

dark energyHubble constant\(f(Q, T)\) gravityequation-of-state parameterPantheon+ data

Mathematics Subject Classification ID

Quantum theory (81-XX) Relativity and gravitational theory (83-XX)

Cites Work

• Modified Chaplygin gas cosmology with statefinder diagnostic in Lyra geometry
• Reconstruction of \(\Lambda\)CDM universe in \(f(Q)\) gravity
• Model-independent reconstruction of \(f(Q)\) non-metric gravity
• First evidence that non-metricity \(f(Q)\) gravity could challenge \(\Lambda\)CDM
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• Reconstruction of \(f(Q,T)\) Lagrangian for various cosmological scenario
• Dark energy constraint on equation of state parameter in the Weyl type \(f(Q,T)\) gravity
• The cosmological constant and dark energy
• ΛCDM epoch reconstruction from F ( R , G ) and modified Gauss–Bonnet gravities
• Cosmological perturbation theory in f(Q,T) gravity
• Gravitation und Elektrizität.
• A new look at the statistical model identification
• Interaction of divergence-free deceleration parameter in Weyl-type \(f(Q, T)\) gravity

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