Accelerating cosmological expansion from shear and bulk viscosity
Stefan Floerchinger1, Nikolaos Tetradis1,2, Urs Achim Wiedemann1
1Physics Department, Theory Unit, CERN, CH-1211 Genève 23, Switzerland.
Physical Review Letters
|March 21, 2015
Abstract:
The dissipation of energy from local velocity perturbations in the cosmological fluid affects the time evolution of spatially averaged fluid dynamic fields and the cosmological solution of Einstein's field equations. We show how this backreaction effect depends on shear and bulk viscosity and other material properties of the dark sector, as well as the spectrum of perturbations. If sufficiently large, this effect could account for the acceleration of the cosmological expansion.
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