# Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology

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## Abstract

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## 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

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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

**AMA Style**

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 Style**

Brevik, 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