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Galaxies 2013, 1(2), 107-113; doi:10.3390/galaxies1020107

Rip Cosmology via Inhomogeneous Fluid

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Received: 31 July 2013 / Revised: 10 August 2013 / Accepted: 12 August 2013 / Published: 15 August 2013
(This article belongs to the Special Issue Cosmology with Fluid Components)
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Abstract: The conditions for the appearance of the Little Rip, Pseudo Rip and Quasi Rip universes in the terms of the parameters in the equation of state of some dark fluid are investigated. Several examples of the Rip cosmologies are investigated.
Keywords: cosmological models; dark fluid; equation of state cosmological models; dark fluid; equation of state
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.

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MDPI and ACS Style

Obukhov, V.V.; Timoshkin, A.V.; Savushkin, E.V. Rip Cosmology via Inhomogeneous Fluid. Galaxies 2013, 1, 107-113.

AMA Style

Obukhov VV, Timoshkin AV, Savushkin EV. Rip Cosmology via Inhomogeneous Fluid. Galaxies. 2013; 1(2):107-113.

Chicago/Turabian Style

Obukhov, Valerii V.; Timoshkin, Alexander V.; Savushkin, Evgenii V. 2013. "Rip Cosmology via Inhomogeneous Fluid." Galaxies 1, no. 2: 107-113.

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