Covariant density and velocity perturbations of the quasi-Newtonian cosmological model in f(T) gravity

Abstract We investigate classes of shear-free cosmological dust models with irrotational fluid flows within the framework of f(T) gravity. In particular, we use the $$1 + 3$$ 1 + 3 covariant formalism and present the covariant linearised evolution and constraint equations describing such models. We...

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Bibliographic Details
Main Authors: Heba Sami, Shambel Sahlu, Amare Abebe, Peter K. S. Dunsby
Format: Article
Language:English
Published: SpringerOpen 2021-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-021-09615-6

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