Dynamics of Linear Scalar Perturbation in f(Q)+f(T) class of f(Q,T) gravity
arXiv:2508.03495 · doi:10.1142/S0217732325501433
Abstract
In this work, we study the f(Q,T) model of symmetric teleparallel modified gravity in the framework of cosmological perturbation theory. Using a general approach, we extract the differential matter density equation then we simplify it as a second-order equation by considering the sub-Hubble approximation. Our analysis is then based on two different forms of f(Q,T) that we study in a classic approach and again using Holographic dark energy. Our initial results yield a significant divergence from the perturbed behavior of the LambdaCDM model, imposing stringent constraints on the feasibility of this class of theories but the HDE contribution triggers an interesting discussion.
References in corpus (31)
- f(R,T) gravity
- A Model of Holographic Dark Energy
- Coincident General Relativity
- Quantum deSitter cosmology and phantom matter
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- The teleparallel equivalent of general relativity
- Cosmology in geometry
- First evidence that non-metricity f(Q) gravity could challenge CDM
- Dynamics of scalar perturbations in f(R,T) gravity
- Signatures of -gravity in cosmology
- On the Importance of NNLO QCD and Isospin-breaking Corrections in
- Black holes in Gravity
- Lagrange formulation of the symmetric teleparallel gravity
- Can gravity challenge CDM?
- gravity models with observational constraints
- New models and Big Bang Nucleosynthesis constraints in gravity
- Baryogenesis in Gravity
- Cosmological Perturbation Theory in Gravity
- Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
- Energy conditions in gravity
- Constraining effective equation of state in gravity
- Accelerating Universe in Hybrid and Logarithmic Teleparallel Gravity
- Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off
- Density Perturbation Growth in Teleparallel Cosmology
- Cosmological Perturbation Theory in Metric-Affine Gravity
- Observational Constraints on Growth Index with Cosmography
- Cosmic Growth in Teleparallel Gravity
- Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
- Holographic F(Q,T) Gravity with Lambert Solution
- Improved model of large-field inflation with primordial black hole production in Starobinsky-like supergravity
- Spatial Dependence of the Growth Factor in Scalar-Tensor Cosmology