Perturbations of Kantowski-Sachs models
Michael Bradley, Mats Forsberg, Zolt\'an Keresztes, L\'aszl\'o \'A., Gergely, Peter K.S. Dunsby

TL;DR
This paper analyzes how small disturbances evolve in Kantowski-Sachs cosmological models with a positive cosmological constant using gauge-invariant covariant methods, covering scalar, vector, and tensor modes.
Contribution
It introduces a harmonic decomposition framework for perturbations in Kantowski-Sachs models, extending previous work to include multiple mode types in a gauge-invariant setting.
Findings
Derived six evolution equations for harmonic coefficients.
Handled scalar, vector, and tensor perturbations without vorticity.
Provided a comprehensive covariant approach for anisotropic cosmologies.
Abstract
Perturbations of Kantowski-Sachs models with a positive cosmological constant are considered in a harmonic decomposition, in the framework of gauge invariant 1+3 and 1+1+2 covariant splits of spacetime. Scalar, vector and tensor modes are allowed, however they remain vorticity-free and of perfect fluid type. The dynamics is encompassed in six evolution equations for six harmonic coefficients.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
