Abstract
The stability of interacting holographic dark energy model is discussed. It is found that for some class of the rate of interaction between dark matter and dark energy, the system has a natural solution where the universe had been decelerating in the beginning but finally settles down to an accelerated phase of expansion.
| Original language | English |
|---|---|
| Article number | 92 |
| Journal | General Relativity and Gravitation |
| Volume | 47 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 28 Aug 2015 |
| Externally published | Yes |
Keywords
- Dark energy
- Dynamical systems
- Holographic principle
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