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...
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 |
Similar Items
-
Quantum and Classical Cosmology in the Brans–Dicke Theory
by: Carla R. Almeida, et al.
Published: (2021-08-01) -
Generalised Brans-Dicke cosmology
by: Holden, Damien James
Published: (2002) -
Cosmological solutions of Brans-Dicke equations with cosmological constant
by: I. Ahmadi-Azar
Published: (2002-12-01) -
Gravitational waves in Brans–Dicke theory with a cosmological constant
by: Hatice Özer, et al.
Published: (2021-04-01) -
The Higgs field and the Jordan Brans Dicke cosmology
by: Onder Dunya, et al.
Published: (2021-01-01)