http://arxiv.org/abs/1412.0837
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 begnning but finally settles down to an acelerated phase of expansion.
N. Roy and N. Banerjee
Wed, 3 Dec 14
38/60
Comments: 8 pages; 5 figures
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