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Dark energy and formation of classical scalar fields

Houri Ziaeepour
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Abstract

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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Houri Ziaeepour. 2006-04-03. Dark energy and formation of classical scalar fields. https://doi.org/10.1063/1.2399699

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