Visualization of cosmological density fluctuations with phase space analysis: case study: Brans–Dicke theory

Abstract Cosmological perturbation theory is a powerful tool to understanding the large-scale structure of the Universe. However, the set of field equations describes the general linear perturbations for the cosmological models is highly nonlinear and coupled where no analytical solution can be foun...

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Bibliographic Details
Main Authors: Amin Salehi, Hossein Farajollahi
Format: Article
Language:English
Published: SpringerOpen 2019-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-6509-2