Galaxies 2013, 1(2), 83-95; doi:10.3390/galaxies1020083
Article

Inhomogeneous Viscous Fluids in a Friedmann-Robertson-Walker (FRW) Universe

Received: 20 May 2013; in revised form: 26 June 2013 / Accepted: 27 June 2013 / Published: 9 July 2013
(This article belongs to the Special Issue Cosmology with Fluid Components)
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract: We give a brief review of some aspects of inhomogeneous viscous fluids in a flat Friedmann-Robertson-Walker Universe. In general, it is pointed out that several fluid models may bring the future Universe evolution to become singular, with the appearance of the so-called Big Rip scenario. We investigate the effects of fluids coupled with dark matter in a de Sitter Universe, by considering several cases. Due to this coupling, the coincidence problem may be solved, and if the de Sitter solution is stable, the model is also protected against the Big Rip singularity.
Keywords: inhomogeneous fluids; viscous fluids; dark matter
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MDPI and ACS Style

Myrzakulov, R.; Sebastiani, L.; Zerbini, S. Inhomogeneous Viscous Fluids in a Friedmann-Robertson-Walker (FRW) Universe. Galaxies 2013, 1, 83-95.

AMA Style

Myrzakulov R, Sebastiani L, Zerbini S. Inhomogeneous Viscous Fluids in a Friedmann-Robertson-Walker (FRW) Universe. Galaxies. 2013; 1(2):83-95.

Chicago/Turabian Style

Myrzakulov, Ratbay; Sebastiani, Lorenzo; Zerbini, Sergio. 2013. "Inhomogeneous Viscous Fluids in a Friedmann-Robertson-Walker (FRW) Universe." Galaxies 1, no. 2: 83-95.

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