Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology
Abstract
:1. Introduction
2. Bounce Cosmology via an Inhomogeneous Fluid
2.1. Exponential Model
2.2. Power-Law Model
2.3. Double Exponential Model
3. Stability of the Solutions
4. Dark Energy Coupled With Dark Matter in Viscous Fluid Cosmology
4.1. Little Rip
4.2. Pseudo Rip
5. Conclusions
Acknowledgments
Conflicts of Interest
References
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Brevik, I.; Timoshkin, A. Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology. Universe 2015, 1, 24-37. https://doi.org/10.3390/universe1010024
Brevik I, Timoshkin A. Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology. Universe. 2015; 1(1):24-37. https://doi.org/10.3390/universe1010024
Chicago/Turabian StyleBrevik, Iver, and Alexander Timoshkin. 2015. "Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology" Universe 1, no. 1: 24-37. https://doi.org/10.3390/universe1010024