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arxiv: astro-ph/0601052 · v2 · submitted 2006-01-03 · 🌌 astro-ph · hep-ph

The Paths of Quintessence

classification 🌌 astro-ph hep-ph
keywords darkenergyfieldmodelsphaseplanescalarstructure
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The structure of the dark energy equation of state phase plane holds important information on the nature of the physics. We explain the bounds of the freezing and thawing models of scalar field dark energy in terms of the tension between the steepness of the potential vs. the Hubble drag. Additionally, we extend the phase plane structure to modified gravity theories, examine trajectories of models with certain properties, and categorize regions in terms of scalar field hierarchical parameters, showing that dark energy is generically not a slow roll phenomenon.

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    Extended analysis of DESI DR2 data confirms robust evidence for dynamical dark energy with phantom crossing preference, stable under parametric and non-parametric modeling.