Open AccessThis article is
- freely available
Rip Cosmology via Inhomogeneous Fluid
Department of Physics and Mathematics, Tomsk State Pedagogical University, Tomsk 634061, Russia
* Author to whom correspondence should be addressed.
Received: 31 July 2013; in revised form: 10 August 2013 / Accepted: 12 August 2013 / Published: 15 August 2013
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
Article StatisticsClick here to load and display the download statistics.
Notes: Multiple requests from the same IP address are counted as one view.
Cite This Article
MDPI and ACS Style
Obukhov, V.V.; Timoshkin, A.V.; Savushkin, E.V. Rip Cosmology via Inhomogeneous Fluid. Galaxies 2013, 1, 107-113.
Obukhov VV, Timoshkin AV, Savushkin EV. Rip Cosmology via Inhomogeneous Fluid. Galaxies. 2013; 1(2):107-113.
Obukhov, Valerii V.; Timoshkin, Alexander V.; Savushkin, Evgenii V. 2013. "Rip Cosmology via Inhomogeneous Fluid." Galaxies 1, no. 2: 107-113.