arXiv · 1212.2360
Generalized Semi-Holographic Universe
Abstract
We study the semi-holographic idea in context of decaying dark components. The energy flow between dark energy and the compensating dark matter is thermodynamically generalized to involve a particle number variable dark component with non-zero chemical potential. It's found that, unlike the original semi-holographic model, no cosmological constant is needed for a dynamical evolution of the universe. A transient phantom phase appears while a non-trivial dark energy-dark matter scaling solution keeps at late time, which evades the big-rip and helps to resolve the coincidence problem. For reasonable parameters, the deceleration parameter is well consistent with current observations. The original semi-holographic model is extended and it also suggests that the concordance model may be reconstructed from the semi-holographic idea.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Hui Li, Hongsheng Zhang, Yi Zhang. 2012-12-11. Generalized Semi-Holographic Universe. https://doi.org/10.1088/0256-307x%2F30%2F8%2F089801
Cite the original work for its findings. Save a collection to share your selection of sources.