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arXiv · hep-ph/0008205

Natural Quintessence?

A. Hebecker·C. Wetterich
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Abstract

We formulate conditions for the naturalness of cosmological quintessence scenarios. The quintessence lagrangian is taken to be the sum of a simple exponential potential and a non-canonical kinetic term. This parameterization covers most variants of quintessence and makes the naturalness conditions particularly transparent. Several ``natural'' scalar models lead, for the present cosmological era, to a large fraction of homogeneous dark energy density and an acceleration of the scale factor as suggested by observation.

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A. Hebecker, C. Wetterich. 2000-08-29. Natural Quintessence?. https://doi.org/10.1016/s0370-2693(00)01339-3

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