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Inhomogeneous viscous fluids in FRW universe and finite-future time singularities

We consider inhomogeneous viscous fluids in flat Friedmann-Robertson-Walker universe. We analyze different kinds of such fluids and investigate the possibility to reproduce the current cosmic acceleration providing a different future evolution with respect to the Cosmological Constant case. In particular, we study the presence of finite-future time singularities. We also discuss a general class of "integrable" viscous fluid models whose bulk viscosities obey to a common differential equation.

preprint2014arXivOpen access
Shynaray MyrzakulRatbay MyrzakulovLorenzo Sebastiani
gr-qc
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Open access3 authors1 topic
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Shynaray MyrzakulRatbay MyrzakulovLorenzo Sebastiani

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