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arxiv: 0902.4037 · v5 · pith:J4J6PW3Jnew · submitted 2009-02-23 · 🌌 astro-ph.CO · gr-qc· hep-ph

Slow-Roll Thawing Quintessence

classification 🌌 astro-ph.CO gr-qchep-ph
keywords quintessenceconditionsderivedequationslow-rollthawingderivestate
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We derive slow-roll conditions for thawing quintessence. We solve the equation of motion of $\phi$ for a Taylor expanded potential (up to the quadratic order) in the limit where the equation of state $w$ is close to -1 to derive the equation of state as a function of the scale factor. We find that the evolution of $\phi$ and hence $w$ are described by only two parameters. The expression for $w(a)$, which can be applied to general thawing models, coincides precisely with that derived recently by Dutta and Scherrer for hilltop quintessence. The consistency conditions of $|w+1|\ll 1$ are derived. The slow-roll conditions for freezing quintessence are also derived.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Assessing observational constraints on dark energy

    astro-ph.CO 2024-05 conditional novelty 6.0

    Quintessence models satisfying NEC everywhere predict the w0 > -1 and w0+wa < -1 sector favored by data, due to an approximate degeneracy in the w(z) = w0 + wa z/(1+z) parameterization.

  2. Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data

    astro-ph.CO 2025-09 unverdicted novelty 3.0

    Quintessence models with standard potentials give only modest improvements over Lambda to DESI data on evolving dark energy, while non-minimal couplings allow temporary phantom behavior but face tight gravity constrai...