Dark energy and formation of classical scalar fields

Details Dark energy and formation of classical scalar fields Dark energy and formation of classical scalar fields

2006-04-03

arxiv.org/abs/hep-ph/0604014v1

AIPConf.Proc.861:1059-1065,2006

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages,2 figures. Proceedings of Einstein 2005 Conference

Scientific paper

10.1063/1.2399699

We present a quintessence model for the dark energy in which the quintessence scalar field is produced by the decay of a super heavy dark matter and gradually condensate to a classical scalar field. This model can explain both the smallness and the latest observations by WMAP for the equation of state of the dark energy which has $w \sim -1.06$. We review both classical and field theoretical treatment of this model and briefly explain the most important parameters for obtaining the observed characteristic of the dark energy.

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