Observational Constraints on Hybrid Scale Factor in f(Q,T)$f(Q,T)$ Gravity with Anisotropic Space‐Time
From MaRDI portal
Publication:6082165
DOI10.1002/andp.202300161arXiv2306.14502MaRDI QIDQ6082165
Unnamed Author, B. Mishra, M. Koussour
Publication date: 29 November 2023
Published in: Annalen der Physik (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2306.14502
Cites Work
- Unnamed Item
- Physics in the real universe: time and spacetime
- Exact spatially homogeneous cosmologies
- Late-time acceleration in \(f(Q)\) gravity: analysis and constraints in an anisotropic background
- First evidence that non-metricity \(f(Q)\) gravity could challenge \(\Lambda\)CDM
- Anisotropic dark energy model with a hybrid scale factor
- ACCELERATING DARK ENERGY MODELS IN BIANCHI TYPE-V SPACETIME
- Cosmological models with a hybrid scale factor in an extended gravity theory
- Viscous Bianchi type I universes in brane cosmology
- Extended gravity cosmography
- Cosmological perturbation theory in f(Q,T) gravity
- Inflationary universe: A possible solution to the horizon and flatness problems
This page was built for publication: Observational Constraints on Hybrid Scale Factor in f(Q,T)$f(Q,T)$ Gravity with Anisotropic Space‐Time