English

Slow-roll k-essence

Cosmology and Nongalactic Astrophysics 2009-09-25 v3 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We derive slow-roll conditions for thawing k-essence with a separable Lagrangian p(X,ϕ)=F(X)V(ϕ)p(X,\phi)=F(X)V(\phi). We examine the evolution of the equation of state parameter, ww, as a function of the scale factor aa, for the case where ww is close to -1. We find two distinct cases, corresponding to X0X \approx 0 and FX0F_X \approx 0, respectively. For the case where X0X\approx0 the evolution of ϕ\phi and hence ww is described by only two parameters, and w(a)w(a) is model-independent and coincides with similar behavior seen in thawing quintessence models. This result also extends to non-separable Lagrangians where X0X\approx0. For the case FX0F_X \approx 0, an expression is derived for w(a)w(a), but this expression depends on the potential V(ϕ)V(\phi), so there is no model-independent limiting behavior. For the X0X \approx 0 case, we derive observational constraints on the two parameters of the model, w0w_0 (the present-day value of ww), and the KK, which parametrizes the curvature of the potential. We find that the observations sharply constrain w0w_0 to be close to -1, but provide very poor constraints on KK.

Cite

@article{arxiv.0906.0628,
  title  = {Slow-roll k-essence},
  author = {Takeshi Chiba and Sourish Dutta and Robert J. Scherrer},
  journal= {arXiv preprint arXiv:0906.0628},
  year   = {2009}
}

Comments

7 pages and 5 figures, typos corrected

R2 v1 2026-06-21T13:09:04.048Z