Talk detail

MG13 - Talk detail

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 Participant

Bradley, Michael

Institution

Dept. of Physics, Umeå University  - Dept. of Physics, Umeå University - Umeå - Umeå - Sweden

Session

TC3

Accepted

Yes

Order

4

Time

15:00 - 15:15

Talk

Oral abstract

Title

Perturbations of Kantowski-Sachs models with a cosmological constant
Co-authors Z. Keresztes, M. Forsberg, M. Bradley, P.K.S. Dunsby, L.Á. Gergely

Abstract

Vorticity-free perturbations of Kantowski-Sachs (KS) models with cosmological constant are considered. These can undergo an anisotropic bounce where the universe changes from a contracting to an expanding phase. A simple argument showing that an isotropic bouncing universe is excluded by observations does not hold for KS models. Hence it is of interest to study the evolution and propagation of perturbations and their possible effects on observables, like the Sachs-Wolfe effect. To do this we use the gauge invariant 1+3 and 1+1+2 covariant splits of spacetime. The perturbations are assumed to be vorticity-free and of perfect fluid type, but otherwise include general scalar, vector and tensor modes. In this case the set of equations can be reduced to six propagation equations for six independent variables.

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