25-29 June 2018
Africa/Johannesburg timezone
General information and Registration for SAIP2018 is handled by Eastern Sun Events at: http://www.saipconference.co.za/ <p> Deadline for papers for the conference proceedings is 28 July 2018

Shear-free Dust Cosmological Models in Gravitational Scalar-Tensor Theories

27 Jun 2018, 12:40
20m
Oral Presentation Track D1 - Astrophysics Astrophysics

Speaker

Ms Heba Abdulrahman (North-West University)

Description

Theoretical physics in general and cosmology in particular have faced some challenges due to the recent observations in cosmology and astronomy, such as the discovery of the accelerated cosmic expansion and the existence of dark matter and dark energy. Einstein’s theory of General Relativity (GR) together with the standard model of cosmology fall short of giving any explanations for these problems. Higher-order gravitational theories such as f(R) and scalar-tensor theories of gravity have been suggested to provide an answer to these shortcomings. In this work, we investigate the cosmological implications of such theories such as the background expansion history as well as the evolution of cosmological density perturbations. We present the equivalence between f(R) and scalar-tensor theories of gravity. Although GR is a generalization of Newtonian gravity in the presence of strong gravitational fields, there is no properly defined Newtonian limit of GR on cosmological scales. Recently, general relativistic quasi-Newtonian cosmologies have been studied in the context of large-scale structure formation and nonlinear gravitational collapse in the late-time universe. This despite the general covariant inconsistency of these cosmological models except in some special cases such as the spatially homogeneous and isotropic, spherically symmetric, expanding FLRW spacetimes. f(R) models have been shown to exhibit more shared properties with Newtonian gravitation than does GR. We investigate the existence and integrability conditions of quasi-Newtonian cosmological spacetimes of classes of shear-free cosmological dust models with irrotational fluid flows in the context of scalar-tensor theories of gravity. We also derive the covariant density and velocity propagation equations of such models and analyse the corresponding solutions to these perturbation equations.

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Amare Abebe
North-West University
amare.abbebe@gmail.com

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Primary author

Ms Heba Abdulrahman (North-West University)

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