Density growth in Kantowski–Sachs cosmologies with a cosmological constant
From MaRDI portal
Publication:2892079
DOI10.1088/0264-9381/29/9/095023zbMath1242.83112arXiv1106.4932OpenAlexW1978676121MaRDI QIDQ2892079
No author found.
Publication date: 18 June 2012
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1106.4932
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (4)
Modified Chaplygin gas in anisotropic universes on the brane ⋮ Final fate of Kantowski–Sachs gravitational collapse ⋮ Density perturbation and cosmological evolution in the presence of magnetic field in \(f(R)\) gravity models ⋮ Dynamical system analysis of Einstein-Skyrme model in a Kantowski-Sachs spacetime
This page was built for publication: Density growth in Kantowski–Sachs cosmologies with a cosmological constant
