English

A new parameter in attractor single-field inflation

Cosmology and Nongalactic Astrophysics 2015-06-17 v2 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We revisit the notion of slow-roll in the context of general single-field inflation. As a generalization of slow-roll dynamics, we consider an inflaton ϕ\phi in an attractor phase where the time derivative of ϕ\phi is determined by a function of ϕ\phi, ϕ˙=ϕ˙(ϕ)\dot\phi=\dot\phi(\phi). In other words, we consider the case when the number of ee-folds NN counted backward in time from the end of inflation is solely a function of ϕ\phi, N=N(ϕ)N=N(\phi). In this case, it is found that we need a new independent parameter to properly describe the dynamics of the inflaton field in general, in addition to the standard parameters conventionally denoted by ϵ\epsilon, η\eta, cs2c_s^2 and ss. Two illustrative examples are presented to discuss the non-slow-roll dynamics of the inflaton field consistent with observations.

Cite

@article{arxiv.1502.04167,
  title  = {A new parameter in attractor single-field inflation},
  author = {Jinn-Ouk Gong and Misao Sasaki},
  journal= {arXiv preprint arXiv:1502.04167},
  year   = {2015}
}

Comments

(v1) 11 pages; (v2) 12 pages, discussions improved including the running, to appear in Physics Letters B

R2 v1 2026-06-22T08:29:31.276Z